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Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites: Proceedings of the ESO Workshop held in Castiglione della Pescaia, Italy, 13–17 September, 2004 PDF

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Preview Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites: Proceedings of the ESO Workshop held in Castiglione della Pescaia, Italy, 13–17 September, 2004

ESO ASTROPHYSICS SYMPOSIA European Southern Observatory ——————————————————— SeriesEditor:BrunoLeibundgut S. Randich L. Pasquini (Eds.) Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites Proceedings of the ESO Workshop held in Castiglione della Pescaia, Italy, 13-17 September, 2004 ABC VolumeEditors SofiaRandich LucaPasquini OsservatoriodiArcetri EuropeanSouthernObservatory LargoE.Fermi,5 Karl-Schwarzschild-Str.2 50125Firenze,Italy 85748Garching,Germany SeriesEditor BrunoLeibundgut EuropeanSouthernObservatory Karl-Schwarzschild-Str.2 85748Garching Germany ISBN-10 3-540-34135-8SpringerBerlinHeidelbergNewYork ISBN-13 978-3-540-34135-2SpringerBerlinHeidelbergNewYork LibraryofCongressControlNumber:2006925844 Thisworkissubjecttocopyright.Allrightsarereserved,whetherthewholeorpartofthematerialis concerned,specificallytherightsoftranslation,reprinting,reuseofillustrations,recitation,broadcasting, reproductiononmicrofilmorinanyotherway,andstorageindatabanks.Duplicationofthispublication orpartsthereofispermittedonlyundertheprovisionsoftheGermanCopyrightLawofSeptember9, 1965,initscurrentversion,andpermissionforusemustalwaysbeobtainedfromSpringer.Violationsare liableforprosecutionundertheGermanCopyrightLaw. SpringerisapartofSpringerScience+BusinessMedia springer.com (cid:1)c Springer-VerlagBerlinHeidelberg2006 PrintedinTheNetherlands Theuseofgeneraldescriptivenames,registerednames,trademarks,etc.inthispublicationdoesnotimply, evenintheabsenceofaspecificstatement,thatsuchnamesareexemptfromtherelevantprotectivelaws andregulationsandthereforefreeforgeneraluse. Typesetting:bytheauthorsandtechbooksusingaSpringerLATEXmacropackage Coverdesign:design&productionGmbH,Heidelberg Printedonacid-freepaper SPIN:11741299 55/techbooks 543210 Preface Ten years after the first ESO Workshop on light elements, and five years after the IAU in conference in Natal (Brazil) on the same subject, we felt that it was time to have a new conference on this topic: a wealth of new observational data have become available from the 8-meter telescopes and in particular from the VLT, and, at the same time, in the last years new theoretical roads have also been inaugurated in the interpretation of the stellar data. It soon became clear,ontheotherhand,thatinordertounderstandtheevolution ofthefragile Li and Be in stars and in the Galaxy, the whole problem of internal mixing in stars must be addressed and understood first, and therefore a large number of elements must be investigated, in many different environments. Adding to this general context the fact that the FLAMES facility at the VLT was offered to the community one year earlier, and that it was starting to produceanimpressivewealthofabundancedataofstarsintheGalaxyandinour neighborhoods, the broad concept of the ESO–Arcetri workshop on “Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites” was built. ThelocationhadtobeinourbelovedToscana,andCastiglionedellaPescaia was immediately identified as an ideal place. To achieve from this initial proposal a full conference, which gathered to- gether from September 13 to 17 more than 150 attendees in a smooth organi- zation, was possible only due to the dedicated work of the conference SOC (J. Andersen,G.Gilmore,G.Meynet,P.Molaro,N.Prantzos,R.Rood,C.Sneden, M. Spite, M. Tosi, and A. Weiss), who contributed to the selection of the main topics and speakers and oversaw the scientific organization of the meeting. Spe- cial thanks go to E. Masini, and P. Bristow, D. Galli, P. Sestito, C. Stoffer, and C. Travaglio who, as part of the LOC, made our stay productive and pleasant, andtoG.PaceandJ.D.doNascimentowhotrainedthemselvesconsiderablyby walkingcontinuouslyduringtheconferencedaystobringthemicrophonestoall the participants of the lively discussions. A special thank goes to M. Felli, who told us all the secrets of the beautiful region around Castiglione della Pescaia. The workshop would not have been possible without the support of ESO and of the Arcetri Observatory, but a successful workshop needs most of all the enthusiastic contribution of all the participants, to whom we are grateful. VI Preface We regret that at least three of our speakers were not able to submit their written contribution, but, due to what is likely a statistical spike, they were quite busy just after the conference in a more fundamental business; we thank them for their participation and we wish all the best to their babies. Arcetri and Garching, Sofia Randich December 2005 Luca Pasquini Contents Part I Abundances in the Thin and Thick Disks Metallicities and α-Abundances in Open Clusters E.D. Friel......................................................... 3 Old Open Clusters as Tracers of Galactic Chemical Evolution: the BOCCE Project A. Bragaglia, M. Tosi .............................................. 9 Chemical Abundances and Mixing in Red Clump Stars of the Galaxy G. Tautvaiˇsiene˙, B. Edvardsson, E. Puzeras, E. Stasiukaitis, I. Ilyin...... 11 Abundance Trends in the Thin and Thick Disks S. Feltzing ........................................................ 13 On the Chemical Abundances of Stars with Giant Planets N.C. Santos....................................................... 19 Observational Constraints on Nucleosynthesis in AGB Stars C. Abia, I. Dom´ınguez, O. Straniero, O. Zamora....................... 23 Advances in Chemical Abundances in Planetary Nebulae M. Perinotto, A. Scatarzi, L. Morbidelli .............................. 27 A Comparison of Methods for Photospheric Abundance Determinations in K-Type Stars L. Affer, G. Micela, T. Morel, J.S. Forcada, F. Favata ................. 31 S/R Ratio in Barium Stars D.M. Allen........................................................ 33 Observations of 3He in Planetary Nebulae D.S. Balser, T.M. Bania, R.T. Rood, W.M. Goss ...................... 35 Chemical Composition and Kinematics of Disk Stars O. Bienaym´e, T. Mishenina, C. Soubiran, V. Kovtyukh, A. Siebert....... 37 VIII Contents Cu and Zn in Thick-Disk and Thin-Disk Stars S. Bisterzo, R. Gallino, M. Pignatari................................. 39 NGC2324: A Relatively Young, Metal-Poor Open Cluster Located Beyond the Perseus Spiral Arm J.J. Claria´, A.E. Piatti, A.V. Ahumada .............................. 41 Fluorine Abundances in the Galaxy K. Cunha, V.V. Smith.............................................. 44 Determination of the Age of the Galactic Thin Disk from Th/Eu Stellar Abundance Ratios E.F. del Peloso, L. da Silva, L.I. Arany-Prado, G.F.P. de Mello ......... 46 CNO Abundances in Giants with Precise Radial Velocity Measurements J.D.Jr. do Nascimento, L. da Silva, J.R. De Medeiros, J. Setiawan, L. Pasquini ....................................................... 48 Oxygen in Metal-Rich Stars: Abundances from [OI] 6300, OI 7771–5 and Near-UV OH A. Ecuvillon, G. Israelian, N.C. Santos, N. Shchukina, M. Mayor, R. Rebolo 50 Ci Non-LTE Spectral Line Formation in Late-Type Stars D. Fabbian, M. Asplund, M. Carlsson ................................ 52 Does the [α/Fe] Abundance Ratio Trend Reverse at Super-Solar Regime? A Test on the Role of Accurate Knowledge of Atmospheric Parameters M.Franchini,C.Morossi,P.diMarcantonio,M.L.Malagnini,M.Chavez, L. Rodriguez-Merino ............................................... 54 Abundances and Ages of the Deconvolved Thin/Thick Disks of the Galaxy P. Girard, C. Soubiran ............................................. 56 Studying Old Open Clusters with Detached Eclipsing Binaries F.Grundahl,S.Meibom,H.Bruntt,H.R.Jensen,J.V.Clausen,S.Frandsen 58 Isotopic Abundances in RGB- and AGB-Stars H.U. K¨aufl, B. Aringer, S. Uttenthaler, J. Hron ....................... 60 Abundance Variations in the Galactic Disk: Planetary Nebulae, Open Clusters and Field Stars W.J. Maciel, R.D.D. Costa ......................................... 62 Some Concerns About the Reliability of LTE Abundance Analyses in Cool, Active Stars T. Morel, G. Micela, F. Favata ...................................... 64 Contents IX Chemo-Dynamical Properties of F-G-K Stars in the −1.0 < [Fe/H] < +0.50 Range C.Morossi,M.Franchini,P.diMarcantonio,M.L.Malagnini,M.Chavez, L. Rodriguez-Merino ............................................... 66 Does Rotation of B Stars Depend on Metallicity? Preliminary Results from GIRAFFE Spectra F. Royer, P. North, C. Melo, J.-C. Mermilliod, E.K. Grebel, J. R. de Medeiros, A. Maeder ....................................... 68 Metallicity in Open Clusters G. Pace, L. Pasquini, P. Fran¸cois, F. Matteucci ....................... 70 Light- and Heavy-Element Abundances from Mid-UV and Optical Spectral Syntheses R.C. Peterson ..................................................... 72 FLAMES Observations of the Star Forming Region NGC 6530 L. Prisinzano, F. Damiani, I. Pillitteri, G. Micela ..................... 74 The “Not-so-MAD” Coronal Abundances of Active Stars J. Sanz-Forcada, F. Favata, G. Micela................................ 76 Fundamental Parameters of B Supergiants S.C. Searle, R.K. Prinja, P. Crowther ................................ 78 High Precision Effective Temperatures and New Abundances for a Large Sample of Disk Stars T.V.Mishenina,C.Soubiran,O.Bienaym´e,V.V.Kovtyukh,S.A.Korotin, T.I. Gorbaneva .................................................... 80 Elemental Abundances in 10 Dwarfs of the Galactic Thick Disk G. Tautvaiˇsiene˙, A. Ivanauskas, M. Grenon, I. Ilyin.................... 82 Part II Abundances in the Spheroidal Component Abundances in the Galactic Bulge B. Barbuy, M. Zoccali, V. Hill, A. Renzini, S. Ortolani, D. Minniti, L. Pasquini, E. Bica, A. Gomez, Y. Momany, J. Mel´endez, A. Alves-Brito..................................................... 87 Abundance Ratios in the Galactic Bulge J.P. Fulbright, R.M. Rich, A. McWilliam ............................. 93 Abundances in Globular Cluster Dwarfs/Subgiants E. Carretta........................................................ 95 X Contents Unraveling the Origins and History of the Outer Halo Cluster System I.I. Ivans ......................................................... 101 Chemical Abundance Inhomogeneities in Globular Cluster Stars J.G. Cohen ....................................................... 103 RedGiantsSurveyinωCen:PreliminaryFLAMESGTOResults E. Pancino........................................................ 107 Galactic Evolution of Carbon and Nitrogen G. Israelian ....................................................... 109 First Stars: Abundance Patterns from O to Zn and Derived SNe Yields in the Early Galaxy R. Cayrel, M. Spite ................................................ 114 Nitrogen in the Early Universe J.A. Johnson, F. Herwig, T.C. Beers, N. Christlieb .................... 120 Abundance of Heavy Elements in Extremely Metal-Poor Stars P. Franc¸ois, R. Cayrel, E. Depagne, M. Spite, V. Hill, F. Spite, B. Plez, T. Beers, F. Primas, J. Andersen, B. Barbuy, P. Bonifacio, P. Molaro, B. Nordstr¨om...................................................... 122 The Chemical Compositions of Carbon-Enhanced Metal-Poor Stars W. Aoki, S.G. Ryan, J.E. Norris, T.C. Beers, N. Christlieb, S. Tsangarides, H. Ando............................................ 124 Lead Stars at Low Metallicity: Observation versus Theory D. Delaude, R. Gallino, S. Cristallo, O. Straniero...................... 126 Sulphur in the Early Ages of the Galaxy E. Depagne, V. Hill, M. Spite, P. Franc¸ois, F. Spite, B. Plez, T.C. Beers, B. Barbuy, R. Cayrel, J. Andersen, P. Bonifacio, B. Nordstro¨m, F. Primas......................................................... 128 Star Clusters in the Galactic Anticenter Stellar Structure: New Radial Velocities & Metallicities P.M. Frinchaboy, R.R. Mun˜oz, S.R. Majewski, E.D. Friel, R.L. Phelps, W.B. Kunkel ...................................................... 130 Abundance Variations in NGC 288, NGC262 and NGC 1851 F. Grundahl, H. Bruntt............................................. 132 Heavy Elements and Chemical Enrichment in Globular Clusters G. James ......................................................... 134

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The field of chemical abundances and internal mixing of elements in stars has made large progress in the last decade. Both a wealth of new observational data and in the last years also the inauguration of new theoretical roads have been the stimulus for this ESO Workshop held in Castiglione della Pe
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