J/ApJ/638/725       Fundamental manifold of spheroids        (Zaritsky+, 2006)

The fundamental manifold of spheroids. Zaritsky D., Gonzalez A.H., Zabludoff A.I. <Astrophys. J., 638, 725-738 (2006)> =2006ApJ...638..725Z 2006ApJ...638..725Z
ADC_Keywords: Models ; Galaxies, spectra Keywords: galaxies: elliptical and lenticular, cD - galaxies: formation - galaxies: fundamental parameters - galaxies: structure Abstract: We present a unifying empirical description of the structural and kinematic properties of all spheroids embedded in dark matter halos. We find that the intracluster stellar spheroidal components of galaxy clusters, which we call cluster spheroids (CSphs) and which are typically 100 times the size of normal elliptical galaxies, lie on a fundamental plane as tight as that defined by elliptical galaxies (rms in effective radius of 0.07) but having a different slope. Description: We obtained spectra of galaxies in the fields of the 12 clusters from Paper I (Gonzalez et al., 2005ApJ...618..195G 2005ApJ...618..195G) with insufficient kinematic data in the literature. We observed those galaxies with the Hydra spectrograph at the CTIO Blanco 4m telescope on the nights of 2003 July 28-31 using the KPGL1 grating, which has 632lines/mm and provides a dispersion of 0.59Å/pixel. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table4.dat 21 447 Measurements Used in Fitting the Fundamental Manifold -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 F5.2 [kpc] logR Log of effective radius 7- 11 F5.2 [km/s] logsig Log of velocity dispersion 13- 17 F5.2 [solLum/pc2] logI Log of mean surface brightness within the effective radius 19- 21 A3 --- Ref [1-6, ] Reference(s) (1) -------------------------------------------------------------------------------- Note (1): References as follows: 1 = This paper 2 = Gonzalez et al. (2005ApJ...618..195G 2005ApJ...618..195G) 3 = Jorgensen et al. (1996MNRAS.280..167J 1996MNRAS.280..167J) 4 = Oegerle & Hoessel (1991ApJ...375...15O 1991ApJ...375...15O) 5 = Geha et al. (2003AJ....126.1794G 2003AJ....126.1794G) 6 = Matkovic & Guzman (2005MNRAS.362..289M 2005MNRAS.362..289M) -------------------------------------------------------------------------------- History: From electronic version of the journal Reference: Gonzalez et al., Paper I 2005ApJ...618..195G 2005ApJ...618..195G
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 26-Sep-2008
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