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VLBA polarimetry monitoring of 3C 111 as a tool to probe AGN jet physics on parsec scales PDF

27 Pages·2017·7.03 MB·English
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Preview VLBA polarimetry monitoring of 3C 111 as a tool to probe AGN jet physics on parsec scales

VLBA polarimetry monitoring of 3C 111 as a tool to probe AGN jet physics on parsec scales T.Beuchert, M.Kadler, M.Perucho, C.Großberger, R.Schulz, I.Agudo, C.Casadio, D.Gabuzda, J.L.Gómez, M.Gurwell, D.Homan, Y.Y.Kovalev, M.L.Lister, S.Markoff, S.N.Molina, A.B.Pushkarev, E.Ros, T.Savolainen, T.Steinbring, C.Thum, J.Wilms 2017 June 15 Polarised Emission from Astrophysical Jets 2017, Ierapetra Fromm et al. (2016) Motivation Roca-Sogorb et al. (2008) Cawthorne et al. (2009) Myserlis et al. (2016) TEMZ model: Marscher (2014); MacDonald & Marscher (2016) RAISHIN code: Mizuno et al. (2006,2011,2015); Gomez et al. (2016) Porth et al. (2011) talks and papers, e.g., by A. Fuentes, C. Fromm, K.I. Nishikawa TobiasBeuchert | PolarisedEmissionfromAstrophysicalJets Motivation Roca-Sogorb et al. (2008) Fromm et al. (2016) Cawthorne et al. (2009) Myserlis et al. (2016) TEMZ model: Marscher (2014); MacDonald & Marscher (2016) RAISHIN code: Mizuno et al. (2006,2011,2015); Gomez et al. (2016) Porth et al. (2011) talks and papers, e.g., by A. Fuentes, C. Fromm, K.I. Nishikawa TobiasBeuchert | PolarisedEmissionfromAstrophysicalJets Previous work Kadler et al. (2008) Perucho et al. (2008) • 10 years, 18 epochs • 7 epochs with polarimetry data • great study of kinematics and jet physics TobiasBeuchert | PolarisedEmissionfromAstrophysicalJets Continued MOJAVE monitoring at 15 GHz time e c n a t s i d • 36 epochs in 5 years • most dense sampling of polarized flux • study complex jet-intrinsic dynamics with polarimetry Beuchert et al., 2017, in prep. TobiasBeuchert | PolarisedEmissionfromAstrophysicalJets l direct measure of d r / steepening 3 mas & s T r B / s = l + n + b (1 ↵) � l d r / 1 2 B r or B r � � / / ↵ 1 ⇠ � n N r with n < 0 >3 mas / Peculiar behavior at 3 mas ⇠ 2 5 10 1.0 1.0 ] s a m . p [ e s pr xi a n r i o 7, aj 1 M 0 2 , . al a t 0.1 0.1 e 1011 1011 t r e h c u e B 1010 1010 ] K [ B T 109 109 b 108 108 2 5 10 Core Distance [mas] TobiasBeuchert | PolarisedEmissionfromAstrophysicalJets s T r B / s = l + n + b (1 ↵) � l d r / 1 2 B r or B r � � / / ↵ 1 ⇠ � n N r with n < 0 >3 mas / Peculiar behavior at 3 mas ⇠ 2 5 10 1.0 1.0 l direct measure of d r ] / s a m steepening & 3 mas . p [ e s pr xi a n r i o 7, aj 1 M 0 2 , . al a t 0.1 0.1 e 1011 1011 t r e h c u e B 1010 1010 ] K [ B T 109 109 b 108 108 2 5 10 Core Distance [mas] TobiasBeuchert | PolarisedEmissionfromAstrophysicalJets Peculiar behavior at 3 mas ⇠ 2 5 10 1.0 1.0 l direct measure of d r ] / s a m steepening & 3 mas . p [ e s pr xi a n r i o 7, aj 1 M 0 2 , . al a t 0.1 0.1 e 1011 1011 t s r T r e B h / c u e s = l + n + b (1 ↵) B 1010 1010 � ] K l [ d r B T / 109 109 1 2 B r or B r � � / / ↵ 1 b 108 108 ⇠ � 2 5 10 n N r with n < 0 Core Distance [mas] >3 mas / TobiasBeuchert | PolarisedEmissionfromAstrophysicalJets see talks, e.g., by T. Savolainen S.N. Molina, Y.K. Ma, T. Hovatta, H. Nagai, A. Pasetto Polarimetry Beuchert et al., 2017, in prep. 5 400 0415+379 2007.1-2012.5 4 ] s P a 200 o m 3 l [ a [ m r C i J z 100 E 2 y e D / d 70 b I e 1 e n v 50 a t m e i t 0 n a ] s l 30 i e t R y -1 20 (a) -2 10 8 6 4 2 0 -2 Relative RA [mas] TobiasBeuchert | PolarisedEmissionfromAstrophysicalJets see talks, e.g., by T. Savolainen S.N. Molina, Y.K. Ma, T. Hovatta, H. Nagai, A. Pasetto Polarimetry Beuchert et al., 2017, in prep. 5 400 0415+379 2007.1-2012.5 4 ] s P a 200 o m 3 l [ a [ m r C i J z 100 E 2 y e D / d 70 b I e 1 e n v 50 a t m e i t 0 n a ] s l 30 i e t R y -1 200 20 150 (a) -2 (((PPPAAA+++999000 ))) ��� ??? 10 8 6 4 2 1000 -2 ] g (((PPPAAA === 666333 ))) e kkk ��� d Relative RA [mas] [ 50 A P A V 0 B E C1/C2 (((PPPAAA 999000 ))) -50 ??? ��� ��� -100 (d) 0 2 4 6 8 Core Distance [mas] TobiasBeuchert | PolarisedEmissionfromAstrophysicalJets

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talks and papers, e.g., by A. Fuentes, C. Fromm, K.I. Nishikawa 109. 108. 1011. 1010. 109. 108. M a jor a x is. [m a s]. Core Distance [mas]. T. B. [K. ].
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