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Preview Monthly Notices of the Royal Astronomical Society 1998: Vol 293-304 Index

Monthly Notices OF THE Royal Astronomical Society VOLUME 301 1998 NOVEMBER 21-— DECEMBER 21] (INCORPORATING ANNUAL INDEX VOLS 293-301) The Board of Editors PROFESSOR M. J. BARLOW, DEPARTMENT OI PHYSICS AND ASTRONOMY, UNIVERSITY COLLEGE LONDON DR R. F. CARSWELL (DEPUTY MANAGING EDITOR), INSTITUTE OF ASTRONOMY, CAMBRIDGI DR J. E. DREW, ASTRONOMY GROUP BLACKETT LABORATORY, IMPERIAI COLLEGE LONDON PROFESSOR A. C. FABIAN FRS (MANAGING EDITOR), INSTITUTE OF ASTRONOMY CAMBRIDGI PROFESSOR M. W. FEAST, DEPARTMENT OF ASTRONOMY, UNIVERSITY OF CAPE TOWN PROFESSOR D. R. FLOWER, DEPARTMENT OF PHYSICS, UNIVERSITY OF DURHAM PROFESSOR D. C. HEGGIE, DEPARTMENT OF MATHEMATICS & STATISTICS, UNIVERSITY OF EDINBURGH DR D. W. HUGHES, DEPARTMENT OI! PHYSICS, UNIVERSITY OF SHEFFIELD PROFESSOR J. C. B. PAPALOIZOU, SCHOOL OIF MATHEMATICAL SCIENCES, QUEEN MARY & WESTFIELD COLLEGE LONDON DR P. A. G. SCHEUER, CAVENDISH LABORATORY, CAMBRIDGI PROFESSOR M. J. WARD, DEPARTMENT OF PHYSICS & ASTRONOMY, UNIVERSITY OF LEICESTER PROFESSOR S. D. M. WHITE, MAX-PLANCK INSTITUT FUR ASTROPHYSIK, GARCHING BEI MUNCHEN Published for the Royal Astronomical Society by Blackwell Science OXFORD LONDON EDINBURGH BOSTON MELBOURNI TOKYO BERLIN VIENNA Mon. Not. R. Astron. Soc. 301 (1998) List of key words used in the annual subject indexes (valid from January 1998) This list is common to Monthly Notices of the Royal nuclear reactions, nucleosynthesis, abundances Astronomical Society, Astronomy and Astrophysics, plasmas and The Astrophysical Journal. In order to ease the polarization search, the key words are subdivided into broad cate- radiation mechanisms: non-thermal gories. No more than six subcategories altogether radiation mechanisms: thermal should be listed for a paper. radiative transfer The subcategories in boldface containing the word relativity ‘individual’ are intended for use with specific astro- scattering nomical objects; these should never be used alone, but shock waves always in combination with the most common names turbulence for the astronomical objects in question. Note that each waves object counts as one subcategory within the allowed limit of six. Astronomical instrumentation, methods and The parts of the key words in italics are for reference techniques only and should be omitted when the key words are entered on the manuscript. atmospheric effects balloons instrumentation: detectors General instrumentation: interferometers book reviews instrumentation: miscellaneous editorials, notices instrumentation: photometers errata, addenda instrumentation: polarimeters extraterrestrial intelligence instrumentation: spectrographs history and philosophy of astronomy methods: analytical miscellaneous methods: data analysis obituaries, biographies methods: laboratory methods: miscellaneous Physical data and processes methods: numerical acceleration of particles methods: observational methods: statistical accretion, accretion discs site testing atomic data space vehicles atomic processes techniques: image processing black hole physics techniques: interferometric chaos techniques: miscellaneous conduction techniques: photometric convection techniques: polarimetric cosmic strings techniques: radar astronomy dense matter techniques: radial velocities diffusion techniques: spectroscopic elementary particles telescopes equation of state gravitation hydrodynamics Astronomical data bases instabilities astrodanta obasmes: imicsceallalneo us line: formation atlases line: identification catalogues line: profiles surveys magnetic fields (magnetohydrodynamics) MHD Astrometry and celestial mechanics masers molecular data astrometry molecular processes celestial mechanics, stellar dynamics © 1998 RAS Index ke words stars: carbon eclipses ephemerides stars: chemically peculiar occultations stars: chromospheres reference systems (stars:) circumstellar matter time Stars: coronae Stars: distances The Sun stars: early-type stars: emission-line, Be Sun: abundances Stars: evolution Sun: activity stars: flare Sun: atmosphere Stars: formation Sun: chromosphere stars: fundamental parameters (classification, Sun: corona colours, luminosities, masses, radii, Sun: evolution temperatures, etc.) Sun: faculae, plages Stars: general Sun: filaments (stars: )H ertzsprung—Russell (HR) diagram Sun: flares stars: horizontal branch Sun: fundamental parameters Stars: imaging Sun: general stars: individual... Sun: granulation Stars: interiors Sun: infrared Stars: kinematics Sun: interior stars: late-type Sun: magnetic fields stars: low-mass, brown dwarfs Sun: oscillations stars: luminosity function, mass function Sun: particle emission stars: magnetic fields Sun: photosphere stars: mass-loss Sun: prominences stars: neutron Sun: radio radiation (stars:) novae, cataclysmic variables Sun: rotation stars: oscillations (including pulsations) (Sun: ) solar—terrestrial relations stars: peculiar (except chemically peculiar) (Sun:) solar wind (stars:) planetary systems (Sun:) sunspots stars: Population II Sun: transition region stars: pre-main-sequence Sun: UV radiation (stars:) pulsars: general Sun: X-rays, gamma-rays (stars:) pulsars: individual:... Stars: rotation Solar system Stars: Stauistics comets: general (stars: ) subdwarts comets: individual:... (stars: ) supergiants Earth (stars:) supernovae: general interplanetary medium (stars:) supernovae: individual:... meteors, meteoroids (stars: variables: ) Cepheids minor planets, asteroids (stars: variables: ) 6 Scuti Moon Stars: variables: other planets and satellites: general (stars:) white dwarts planets and satellites: individual... stars: Wolf—Rayet Solar system: formation Solar system: general Interstellar medium (ISM), nebulae ISM: abundances Stars ISM: atoms stars: abundances ISM: bubbles Stars: activity ISM: clouds stars: AGB and post-AGB (1SM:) cosmic rays stars: atmospheres (1SM:) dust, extinction (stars:) binaries (including multiple): close ISM: general (stars:) binaries: eclipsing ISM: globules (stars:) binaries: general (1SM:) Hui regions (stars:) binaries: spectroscopic ISM: individual... (stars:) binaries: symbiotic (except planetary nebulae) (stars:) binaries: visual ISM: jets and outflows (stars:) blue stragglers ISM: kinematics and dynamics © 1998 RAS Index key words ISM: magnetic fields galaxies: photometry ISM: molecules (galaxies: )q uasars: absorption lines (1SM:) planetary nebulae: general (galaxies: )q uasars: emission lines (1SM:) planetary nebulae: individual:... (galaxies: )q uasars: general (1SM:) reflection nebulae (galaxies:) quasars: individual... ISM: structure galaxies: Seyfert (1SM:) supernova remnants galaxies: spiral galaxies: starburst The Galaxy galaxies: star clusters galaxies: statistics Galaxy: abundances galaxies: stellar content Galaxy: centre galaxies: structure Galaxy: evolution Galaxy: formation Cosmology Galaxy: fundamental parameters Galaxy: general (cosmology: ) cosmic microwave background (Galaxy:) globular clusters: general cosmology: miscellaneous (Galaxy:) globular clusters: individual... cosmology: observations Galaxy: halo cosmology: theory Galaxy: kinematics and dynamics (cosmology: ) dark matter (Galaxy: ) open clusters and associations: general (cosmology: ) diffuse radiation (Galaxy: )o pen clusters and associations: individual:... (cosmology: ) distance scale (Galaxy: ) solar neighbourhood (cosmology:) early Universe Galaxy: stellar content (cosmology: ) gravitational lensing Galaxy: structure (cosmology: ) large-scale structure of Universe Galaxies Sources as a function of wavelength galaxies: abundances gamma-rays: bursts galaxies: active gamma-rays: observations (galaxies:) BL Lacertae objects: general gamma-rays: theory (galaxies:) BL Lacertae objects: individual:... infrared: galaxies galaxies: clusters: general infrared: general galaxies: clusters: individual:... infrared: ISM: continuum galaxies: compact infrared: ISM: lines and bands (galaxies:) cooling flows infrared: Solar system galaxies: distances and redshifts infrared: stars galaxies: elliptical and lenticular, cD radio continuum: galaxies galaxies: evolution radio continuum: general galaxies: formation radio continuum: ISM galaxies: fundamental parameters radio continuum: Solar system (classification, colours, luminosities, masses, radii, etc.) radio continuum: stars galaxies: general radio lines: galaxies galaxies: haloes radio lines: general galaxies: individual... radio lines: ISM galaxies: interactions radio lines: Solar system (galaxies: ) intergalactic medium radio lines: stars galaxies: ISM ultraviolet: galaxies galaxies: irregular ultraviolet: general galaxies: jets ultraviolet: ISM galaxies: kinematics and dynamics ultraviolet: Solar system (galaxies:) Local Group ultraviolet: stars galaxies: luminosity function, mass function X-rays: bursts (galaxies:) Magellanic Clouds X-rays: galaxies galaxies: magnetic fields X-rays: general galaxies: nuclei X-rays: ISM galaxies: peculiar X-rays: stars ‘ 1998 R AS Mon. Not. R. Astron. Soc. 293—301 (1998) Subject index General Observations of the SW Sextantis star UU Aquarii (Hoard D.W.., Still M.D., Szkody P., Smith R.C., Buckley D.A.H.), 294, 689 Editorials, notices Global solutions of adiabatic accretion flows with isothermal shocks in Editorial: submission of accepted papers in I pX/L* I px by FTP, 295, Kerr black hole geometry (Lu J.-F., Yuan F.), 295, 66 4 ASCA X-ray observations of EX Hya: spin-resolved spectroscopy (Allan A., Hellier C., Beardmore A.), 295, 167 Errata, addenda Polarimetry of QQ Vul (Cropper M.), 295, 353 Erratum: Paramagnetic alignment of thermally rotating dust (Lazarian Radiation-driven winds from luminous accretion discs (Proga D \.), 293, 208 Stone J.M., Drew J.E.), 295, 595 Erratum: Spiral structure in the accretion disc of the binary IP Pegasi Supersonic wind accretion in massive close binary systems: a 3D (Steeghs D., Harlaftis E.T., Horne K.), 296, 463 SPH simulation of Cen X-3 (Lanzafame G., Belvedere G.), 295, 618 Erratum: Collapse of a radiating star with shear (Chan R.), 299, 811 Erratum: Metallicity and photospheric abundances in field K and M Multiwavelength monitoring of GRS 1915 + 105 (Bandyopadhyay R.., dwarts (Zboril M., Byrne P.B., Rolleston W.R.J.), 301, 1104 Martini P., Gerard E., Charles P.A., Wagner R.M., Shrader C., Shahbaz T., Mirabel I.F.), 295, 623 Polarimetry of the eclipsing polar RX JO929.1—2404 (Buckley D.A.H., Ferrario L., Wickramasinghe D.T., Bailey J.A.), 295, 899 Physical data and processes On the outburst amplitude of the soft X-ray transients (Shahbaz T.., Kuulkers E.), 295, L1 Acceleration of particles Spiral shocks in accretion discs (Godon P., Livio M., Lubow S.), 295, The Deutsch field gamma-ray pulsar — IJ. Application of the model Lil (Higgins M.G., Henriksen R.N.), 295, 188 On the orbital period distribution of cataclysmic variables (Hellier C., Naylor T.), 295, L50 Accretion, accretion discs 3+ 1 formulation of non-ideal hydrodynamics (Peitz J., Appl S.), 296, Polarization from magnetized accretion discs — II. The effects of 231 absorption opacity on Faraday rotation (Agol E., Blaes O., lonescu Gamma-ray bursts from internal shocks in a relativistic wind: temporal Zanetti C.), 293, | and spectral properties (Daigne F., Mochkovitch R.), 296, 275 Nova V1425 Aquilae 1995: the early appearance of accretion Impact of small bodies on to discs around compact objects — Il processes in an intermediate polar candidate (Retter A., Leibowitz Interaction with the disc (Landry S., Pineault S.), 296, 359 E.M., Kovo-KaritiO .), 293, 145 Discovery of the high-field polar RX J1724.0 + 4114 (Greiner J., White dwarf masses in magnetic cataclysmic variables: multi Schwarz R., Wenzel W.), 296, 437 temperature fits to Ginga data (Cropper M., Ramsay G., Wu K.), Erratum: Spiral structure in the accretion disc of the binary IP Pegasi 293, 222 (Steeghs D., Harlaftis E.T., Horne K.), 296, 463 Limits from rapid TeV variability of Mrk 421 (Celotti A., Fabian A.C., rhe mass of the white dwarf in the old nova BT Mon (Smith D.A., Dhillon V.S., Marsh T.R.), 296, 465 Rees M.J.), 293, 239 rhe biconical kiloparsec structure generated by nuclear starbursts A radiation-driven disc wind model for massive young stellar objects (Tenorio-TagleG ., Muitoz-Tunén C.), 293, 299 (Drew J.E., Proga D., Stone J.M.), 296, L6 \ note on the conditions for SSD-ADAF transitions (Abramowicz Predicting the future of superhumps in classical nova systems (Rettet M.A., Igumenshchev I.V., Lasota J.-P), 293, 443 A., Leibowitz E.M.), 296, L37 Stellar capture by an accretion disc (Vokrouhlicky D., Karas V.), 293, Outbursts of irradiated accretion discs (King A.R.), 296, L45 LI Hot accretion discs with thermal Comptonization and advection in \pparent superluminal expansion in Cygnus X-3 (Newell S.J., Garrett luminous black hole sources (Zdziarski A.A.), 296, L51 M.A., Spencer R.E.), 293, L17 Waves and instabilities in a differentially rotating disc containing a The light curves of soft X-ray transients (King A.R., Ritter H.), 293, poloidal magnetic field (Ogilvie G.I.), 297, 291 L42 Simulations of superhumps and superoutbursts (Murray J.R.), 297, 323 The ultraviolet spectrum of the narrow-line Seyfert | galaxy RE The changing X-ray light curves of the intermediate polar FO Aquarii J1034+396 (Puchnarewicz E.M., Mason K.O., Siemiginowska A.), (Beardmore A.P., Mukai K., Norton A.J., Osborne J.P., Hellier C.), 293, L52 297, 337 RX J1914.4 + 2456: the first double-degenerate polar? (Cropper M.., Soft X-ray transients in the Hertzsprung gap (Kolb U.), 297, 419 Harrop-Allin M.K., Mason K.O., Mittaz J.P.D., Potter S.B., Ramsay Iron Ka linewidths in magnetic cataclysmic variables (Hellier C., G.), 293, LS7 Mukai K., Osborne J.P.), 297, 526 Fast variability of the outflow in the Z CMa system (Chochol D., A general relativistic calculation of boundary layer and disc luminosity Teodorani M., Strafella F., Errico L., Vittone A.A.), 293, L73 for accreting non-magnetic neutron stars in rapid rotation (Thampan he circumnuclear material in the Galactic Centre: a clue to the A.V., Datta B.), 297, 570 accretion process (Sanders R.H.), 294, 35 Super-Eddington accretion discs around Kerr black holes RX J0744—S2: a probable new intermediate polar (Ramsay G., (Beloborodov A.M.), 297, 739 Buckley D.A.H., Cropper M.), 294, 187 Photon bubbles in accretion discs (Gammie C.F.), 297, 929 Magnetic and vertical shear instabilities in accretion discs (Urpin V.., On the absence of jet features in the optical spectra of cataclysmic Brandenburg A.), 294, 399 variables (Knigge C., Livio M.), 297, 1079 The radio—optical correlation in steep-spectrum quasars (Serjeant S.., The runaway instability of self-gravitating tori with non-constant Rawlings S., Maddox S.J., Baker J.C., Clements D., Lacy M., Lilje specific angular momentum around black holes (Masuda N., Nishida P.B.), 294, 494 S., Eriguchi Y.), 297, 1139 Effects of the Blandford—Znajek process on the evolution of the central ‘Stokes imaging’ of the accretion region in magnetic cataclysmic black holes of accretion discs (Wang D.X., Lu Y., Yang L.T.), 294, variables — I. Conception and realization (Potter S.B., Hakala P.J., 667 Cropper M.), 297, 1261 © 1998 RAS Subject index ymparison of white dwarf mass estimators using the intermediate Magnetospheric accretion and pre-main-sequence stellar masses polar XY Ari (Ramsay G., Cropper M., Hellier C., Wu K.), 297, (Bonnell 1.A., Smith K.W., Meyer M.R., Tout C.A., Folha D.F.M | hy Emerson J.P.), 299, 1013 . Simulations of spiral structure in the accretion disc of IP Pegasi during Radiatively driven mass accretion on to galactic nuclei by outburst (Armitage P.J.. Murray J.R.), 297, L81 circumnuclear starbursts (Umemura M., Fukue J., Mineshige S.) Stellar dynamics in a galactic centre surrounded by a massive accretion 299, 1123 ian description (Vokrouhlicky D., Karas V.), 298, Eccentric instability of a two-dimensional fluid disc with a central massive object (Taga M., lye M.), 299, 1132 structure around a magnetic neutron star: analytic and Magnetic reconnection: flares and coronal heating in active galactic solutions (Brandenburg A., Campbell C.G.), 298, nuclei (Di Matteo T.), 299, L15 On the precession of accretion discs in X-ray binaries (Larwood J.) u of Ha flares in AE Aquarii (Welsh W.F., Horne K 299, L32 298, 285 Echoes from an irradiated disc in GRO J1655—40 (Hynes R.L., O’ Brien ervation of Cygnus X-1 — L. Spectral analysis (Dove J.B K., Horne K., Chen W., Haswell C.A.), 299, L37 ns J.. Nowak M.A., Vaughan B.A., Begelman M.C.), 298, 729 Variability associated with @ accretion disc theory for standard ibsorption and reflection of a multitemperature advection-dominated discs (Blackman E.G.), 299, L48 tron—bremsstrahlung X-ray cooling shock in BY Cam (Done Three-dimensional numerical simulation of gaseous flow structure in Maed7ziarz P.) 298, }3 semidetached binaries (Bisikalo D.V., Boyarchuk A.A., Chechetkin aX isymmetric relativistic Bondi—Hoyle accretion on toa V.M., Kuznetsov O.A., Molteni D.), 300, 39 Schwarzschild black hole (Font J.A., Ibafiez J.M.), 298, 835 The 1996 outburst of GRO J1655—40: the challenge of interpreting the Instability of spherical accretior 1. Shock-free Bondi accretion multiwavelength spectra (Hynes R.I., Haswell C.A., Shrader C.R Kovalenko I.G., Eremin M.A.), 298, 861 hen W., Horne K., Harlaftis E.T., O’ Brien K., Hellier C., Fender imit-cycle behaviour of thermally unstable accretion flowson to R.P.). 300, 64 black holes (Szuszkiewicz E., Miller J.( 298, 888 Magnetic field bending in accretion discs with dynamos (Campbell Yu ion disc outbursts: a new version of an old model (Hameury C.G., Papaloizou J.C.B., Agapitou V.), 300, 315 J.-M., Menou K., DubusG ., Lasota J.-P., Huré J.-M.), 298, 1048 Tilted accretion discs in cataclysmic variables: tidal instabilities and Slim accretion discs: a model for ADAF-—SLE transitions superhumps (Murray J.R., Armitage P_J.), 300, 561 1.V., Abramowicz M.A., Novikov I1.D.), 298, 1069 An RXTE observation of the Seyfert | galaxy MCG—6-30-15: X-ray d spectra of the accretion disc and gas stream of reflection and the iron abundance (Lee J.C., Fabian A.C., Reynolds iiable UX Ursae Majoris (Baptista R., Horne K C.S., lwasawa K., Brandt W.N.), 300, 583 Hubeny I., Long K.S., Rutten R.G.M.), 298, 1079 On spin-up/spin-down torque reversa mdi : reting nulsars ( cataclysmic variable period gap: still there (Kolb U., King A.R.., Wickramasinghe D.T.), 300, 1015 Ritter H.), 298, L29 An ‘outside-in’ outburst of Aql X-1 (Shahbaz T., Bandyopadhyay Magnetic torques between ! m discs and stars (Torkelsson U.) R.M., Charles P.A., Wagner R.M., Muhli P., Hakala P., Casares J 298, L55 Greenhill J.), 300, 1035 Disc structure around s ¥ Magnetic accretors: a full disc solution Numerical simulations of protostellar encounters — I. Star—disc vith turbulent diffusivity umpbell C.G., Heptinstall P.M.), 299, encounters (Boffin H.M.J., Watkins S.J., Bhattal A.S., Francis N Whitworth A.P.), 300, 1189 olution of neutron stars uigh-mass ray binaries (Urpin V Numerical simulations of protostellar encounters — Il. Coplanar Konenkov D., Geppert U.), 299, disc—dise encounters (Watkins S.J., Bhattal A.S., Boffin H.M.J The new intermediate polar RX J1238—38: a system below the period Francis N., Whitworth A.P.), 300, 1205 zap? (Buckley D.A.H.., ¢ per M., RamsayG ., Wickramasinghe Numerical simulations of protostellar encounters — III. Non-coplanar D.T.), 299, 83 disc—dise encounters (Watkins S.J., Bhattal A.S., Boffin H.M.J ltrasoft X-ray components high-temperature extreme Francis N., Whitworth A.P.), 300, 1214 Puchnarewicz E.M.), 299, [ron line profiles including emission from within the innermost stable Phase-resolved Hubble Space Telescope ultraviolet spectroscopy of orbit of a black hole accretion disc (Young A.J., Ross R.R., Fabian V 795 Her (Rosen S.R., Prinja R.K., Drew J.E., Mason K.O., Howell A.C.), 300, L111 S.B.), 299, 305 On the spia paradigm and the radio dichotomy of quasars (Moderski X-ray spectroscoy the broad-line radio galaxy 3C 111 (Reynold R., Sikora M., Lasota J.-P.), 301, 142 C.S., lwasawa K., Crawford C.S., Fabian A.C.), 299, 410 \ spectral decomposition of the variable optical, ultraviolet and X-ray Comptonization and QPO origins in accreting neutron star systems continuum of NGC 5548 (Magdziarz P., Blaes O.M., Zdziarski (Lee H.( Miller G.S.), 299, 479 4.A., Johnson W.N., Smith D.A.), 301, 179 Evidence for a rotational velocity field about the white dwarf of V347 The orbital period of HDE 226868/Cyg X-1 (LaSala J., Charles P.A Puppis (Sull M.D., Buckley D.A.H., Garlick M.A.), 299, 545 Smith R.A.D., Batuciriska-Church M., Church M.J.), 301, 285 Spectroscopic evidence for two-pole accretion in the intermediate Soft X-ray transient light curves as standard candles: exponential polar RX JOS558 + 5353 (Sull M.D., Duck S.R., Marsh T.R.), 299, versus linear decays (Shahbaz T., Charles P.A., King A.R.), 301, 59 382 rhe stream impact region in the disc of WZ Sge (Spruit H.C., Rutten Broad-band * -ray/y-ray spectra and binary parameters of GX 339-4 R.G.M.), 299, 768 and their astrophysical implications (Zdziarski A.A., Poutanen J., Smoothed particle hydrodynamic simulations of viscous accretion Mikotajewska J., Gierliriski M., Ebisawa K., Johnson W.N.), 301, discs around black holes (LanzafameG ., Molteni D., Chakrabarti 435 S.K.), 299, 799 Disc structure around strongly magnetic accretors: a full disc solution X-ray confirmationo f the new intermediate polar RX J1238—38 with buoyancy diffusivity (Campbell C.G., Heptinstall P.M.), 301, (Hellier C., Beardmore A.P., Buckley D.A.H.), 299, 851 558 Oscillatory instability of radiative shocks with mulitiple cooling Stream overflow and dwarf nova eruptions (Schreiber M.R., Hessman processes (Saxton C.J.. Wu K., Pongracic H., Shaviv G.), 299, 862 F.V.), 301, 626 4 double-frequency dwarf nova oscillation in OY Car (Marsh T.R., The chemical evolution of the secondary stars in close binaries, arising Horne K.), 299, 921 from common-envelope evolution and nova outbursts (Marks P.B., \ ROSAT observation of the dipping, flaring and eclipsing polar MN Sarna M.J.), 301, 699 Hya (RX J0929. |—2404) (Buckley D.A.H., Barrett P.E., Haber! F.. Emission-line profiles from self-gravitating toroids around black holes Sekiguchi K.), 299, 998 (Usui F., Nishida S., Eriguchi Y.), 301, 721 © 1998 RAS Subject index An analytic model for disc disruption by strong stellar magnetic fields Super-Eddington accretion discs around Kerr black holes (( ampbell ¢ G.), 301, 754 (Beloborodov A.M.), 297, 739 Supermassive black holes in early-type galaxies: relationship with Atomic data radio emission and constraints on the black hole mass function Emission lines of [Ne tv] in the optical and ultraviolet spectrao f (Franceschini A., Vercellone S., Fabian A.C.), 297, 817 gaseous nebulae (Keenan F.P., Aller L.H., Bell K.L., Espey B.R The runaway instability of self-gravitating tori with non-constant Feibelman W.A., Hyung S., McKenna F.C., Ramsbottom C.A.) specific angular momentum around black holes (Masuda N., Nishid: 295, 683 S., Eriguchi Y.), 297, 1139 The broadening of d—f and f—d transitions by collisions with neutral Non-axisymmetric relativistic Bondi—Hoyle accretion on toa hydrogen atoms (Barklem P.S., O° Mara B.J.. Ross J.E.), 296, 1057 Schwarzschild black hole (Font J.A., [baéfiez J.M.). 298, 835 Solar EUV line identifications from delayed beam-foil spectra (Trabert Orbital motion of a massive object in a dense stellar system (Taga M E.) 297. 399 lye M.), 299, 111 UV transitions of astrophysical interest in Ge, As 1 and Se 1 (Biémont Smoothed particle hydrodynamic simulations of viscous accretion E., Morton D.C., Quinet P.), 297, 713 discs around black holes (Lanzafame G., Molteni D., Chakrabarti The WC 10 central stars CPD—56° 8032 and He 2-113 — III. Wind S.K.), 299, 799 electron temperatures and abundances (De Marco O., Storey P.J., Radiatively driven mass accretion on to galactic nuclei by Barlow M.J.), 297, 999 circumnuclear starbursts (Umemura M., Fukue J., Mineshige S.) Recombination of helium-like ions — I. Photoionization cross-sections 299, 1123 and total recombination and cooling coefficients for atomic helium Resonant tidal disruption in galactic nuclei (Rauch K.P., Ingalls B.), (Hummer D.G.., Storey P.J.), 297, 1073 299, 1231 Precise laboratory wavelengths of the Mgi and Mg ti resonance High-redshift galaxies, their active nuclei and central black holes transitions at 2853, 2803 and 2796 A (Pickering J.C., Thorne A.P (Haehnelt M.G., Natarajan P., Rees M J.), 300, 817 Webb J.K.), 300, 131 Iron line profiles including emission from within the innermost stable Accurate free—free Gaunt factors for astrophysical plasmas (Sutherland orbit of a black hole accretion disc (Young A.J., Ross R.R., Fabian R.S.), 300, 321 A.C.), 300, L11 The 3s -S—4p -P® transition probability in Mg u (Fleming J., Hibbert A On the spin paradigm and the radio dichotomy of quasars (Moderski Bell K.I Vaeck N.), 300, 767 R., Sikora M., Lasota J.-P.), 301, 142 The broadening of strong lines of Ca*, Mg* and Ba* by collisions Emission-line profiles from self-gravitating toroids around black holes with neutral hydrogen atoms (Barklem P.S., O° Mara B.J.), 300, (Usui F., Nishida S., Eriguchi Y.), 301, 721 863 Photoionization from excited states of Ne1 (Seaton M.J.), 300, L1 Chaos Anomalous mixing of the w -P°, and x °P®, levels in Fe | (Donnelly Lattice dynamical system modelling of molecular clouds (Rousseau M.P.. Hibbert A.), 301, 809 G., Chaté H., Le Bourlot J.), 294, 373 Intermittent behaviour in axisymmetric mean-field dynamo models in Atomic processes spherical shells (Tworkowski A., Tavakol R., Brandenburg A Effective collision strengths for fine-structure forbidden transitions Brooke J.M., Moss D., Tuominen I.), 296, 287 among the 2s-2p° levels of Ne tv (Ramsbottom C.A., Bell K.1 Modulation and symmetry changes in stellar dynamos (Knobloch f Keenan F.P.), 293, 233 Tobias S.M.. Weiss N.O.), 297, 1123 Electron impact excitation of the ground-state ’P fine-structure levels Three-body dynamics: intermittent chaos with strange attractor in atomic oxygen (Bell K.L., Berrington K.A., Thomas M.R.J.), 293, (Heinaimaki P., Lehto H.J., Valtonen M.J., Chernin A.D.), 298, 790 L83 \ two-layer aw-dynamo model with dynamic feedback on the w-effect H.,, formation on interstellar grains tn different physical regimes (Roald C.B.), 300, 397 (Biham O., Furnam I., Katz N., Pirronello V., Vidali G.), 296, 869 Phase mixing in time-independent Hamiltonian systems (Kandrup UV transitions of astrophysical interest in Ge 1, Asti and Se 1 (Biémont H.E.), 301, 960 E., Morton D.C., Quinet P.), 297, 713 Recombinationo f helium-like ions — I. Photoionization cross-sections Conduction and total recombination and cooling coefficients for atomic helium Self-inhibiting heat flux (Pistinner S.L., Eichler D.), 301, 49 (Hummer D.G.., Storey P.J.), 297, 1073 Accurate free—free Gaunt factors for astrophysical plasmas (Sutherland Convection R.S.), 300, 321 4 note on the conditions for SSD—ADAF transitions (Abramowicz M.A., lgumenshchev I. V., Lasota J.-P), 293, 443 Black hole physics \ numerical simulation of supersonic thermal convection (Dyt C.P The radio—optical correlation in steep-spectrum quasars (Serjeant S Prentice A.J.R.), 296, 56 Rawlings S.. Maddox S.J., Baker J.C., Clements D.. Lacy M., Lily Evolution of DA white dwarfs in the context of a new theory of P.B.), 294, 494 convection (Althaus L.G., Benvenuto O.G.), 296, 206 Effects of the Blandford—Znajek process on the evolution of the central On the validity of quasi-linear kinematic mean-field electrodynamics black holes of accretion discs (Wang D.X., Lu Y., Yang L.T.), 294, in astrophysical flows (Petrovay K., Zsarg6 J.), 296, 245 667 Evolutionary sequences for Nova V1974 Cygni using new nuclear On the magnetohydrodynamic description of a two-component plasma reaction rates and opacities (Starrfield S., Truran J.W., Wieschet in the Kerr metric (Khanna R.), 294, 673 M.C., Sparks W.M.), 296, 502 Are Q-stars a serious threat for stellar-mass black hole candidates? The dependence of the diffusion coefficient on the mixing length in (Miller J.C., Shahbaz T., Nolan L.A.), 294, L25 Kato’s overstable zone (Umezu M.), 298, 193 Global solutions of adiabatic accretion flows with isothermal shocks in Stellar evolution models for Z = 0.0001 to 0.03 (Pols O.R., Schrédet Kerr black hole geometry (Lu J.-F., Yuan F.), 295, 66 K.-P., Hurley J.R., Tout C.A., Eggleton P.P.), 298, 525 Generation of magnetic fields by a gravitomagnetic plasma battery Effectso f errors in the solar radius on helioseismic inferences (Basu (Khanna R.), 295, L6 S.), 298, 719 3+ 1 formulation of non-ideal hydrodynamics (Peitz J., App! S.), 296, Solar p-mode excitation: further insight from recent low-/ BiSON 231 helioseismological data (Chaplin W.J., Elsworth Y., Isaak G.R.., Hot accretion discs with thermal Comptonization and advection in Lines R., McLeod C.P., Miller B.A., New R.), 298, L7 luminous black hole sources (Zdziarski A.A.), 296, L51 Modelling photospheric magnetoconvection (Blanchflower S.M., Soft X-ray transients in the Hertzsprung gap (Kolb U.), 297, 419 Rucklidge A.M., Weiss N.O.), 301, 593 1998 RAS Subje f index 1e-dimensional magnetized relativistic pai s (Marks P.B M.), 293, 44 M 1. yf artificia ity on a hydrodynamic mode M.. Ishid Tanaka 294, 224 Cosmic strings Metal enrichment « wctic medium (Gnedin N.Y.), 294, 407 Global solutions o atic accretion flows with isothershmocaksl i n Kerr black hok ymetry (Lu J.-F.. Yuan F.), 295, 66 4 cosmological h “dynamic code based on the piecewise parabolic Dense matter method (Gheller Pantano O., Moscardini L.), 295,519 Radiation-driven winds from luminous accretion discs (Proga D Stone J.M., Dr 295, 595 lose binary systems: a 3D SPH me G., Belveder ), 295, 618 ooling resulting trom luminous Diffusion tuko N Habe \ sibasi N 295, cular clump 295, 738 Im )possiDi« io M., I Hydrodynamiofc sth e .Y., Hui L.), 296, 44 Elementary particles Equation of state tion disc of the ‘> K.), 296, 463 ‘A Gravitation ised by 1 J.M., O’Brein T.J., Bode M.I ul lel for massive 1.M.), 296, L6 ri oO c DM hydrodynamical P B., Dominguez-T eiro R.), 297, 177 Stabilit } lifferentially rotati G.1.}, 297, 291 perhumps and superoutbursts (Murray J.R.) 297, 323 yn to th e hypersonic, radiative blunt body problem 297. ~ 4 convenient set of comoving cosmological variables and thei ipplication (Martel H., Shapiro P.R.), 297, 46 Super-Eddington accretion discs around Kerr black hol (Beloborodov A.M.), 297, 739 Galaxy formation and evolution — |. The Padua (CarraroG ., Lia ¢ iosi C.), 297, 1021 Pattern speed of the stellar bar in NGC 7479 (Laine S., Shlosman | Heller C.H.), 297, 1052 The large-scale structure of FR-II radio sources (Komis Falle S.A.E.G.), 297, 108 The low-redshift evolution of the an-a { eun I eonard Montero M.), 301, 4... Efstathiou G.), 297, L49 Simulations of spiral structure in the accretion disc of IP Pegasi during outburst (Armitage P.J.. Murray J.R.), 297, L81 Cometary and bipolar ultracompact H 1 regions (Redman M.P tructul nerated Dy nuciear starDursts Williams R.J.R., Dyson J.E.), 298, 33 Mufioz-Tufién ¢ 293, 299 Numerical simulationso f rotating cooling flows in galaxy cluster 4 note on the conditions for SSD—ADAF transitions (Abramowicz environments (Garasi C., Loken C., Burns J.0., Roettiger K.), 298, M.A.., Igumenshchev 1.V ., Lasota J.-P), 293, 443 697 1998 RAS

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