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J/MNRAS/416/1680    ATLAS3D project. VII.                   (Cappellari+, 2011)

The ATLAS3D project. VII. A new look at the morphology of nearby galaxies: the kinematic morphology-density relation. Cappellari M., Emsellem E., Krajnovic D., McDermid R.M., Serra P., Alatalo K., Blitz L., Bois M., Bournaud F., Bureau M., Davies R.L., Davis T.A., de Zeeuw P.T., Khochfar S., Kuntschner H., Lablanche P.-Y., Morganti R., Naab T., Oosterloo T., Sarzi M., Scott N., Weijmans A.-M., Young L.M. <Mon. Not. R. Astron. Soc., 416, 1680-1696 (2011)> =2011MNRAS.416.1680C
ADC_Keywords: Surveys ; Galaxy catalogs ; Morphology Keywords: galaxies: elliptical and lenticular, cD - galaxies: evolution - galaxies: formation - galaxies: kinematics and dynamics - galaxies: structure Abstract: In Paper I of this series we introduced a volume-limited parent sample of 871 galaxies from which we extracted the ATLAS3D sample of 260 early-type galaxies (ETGs). In Papers II and III we classified the ETGs using their stellar kinematics, in a way that is nearly insensitive to the projection effects, and we separated them into fast and slow rotators. Here we look at galaxy morphology and note that the edge-on fast rotators generally are lenticular galaxies. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 46 260 The local galaxy density for the ATLAS3D sample of 260 early-type galaxies table3.dat 46 611 The local galaxy density for the 611 spiral galaxies in the ATLAS3D parent sample
See also: J/MNRAS/413/813 : ATLAS3D project. I. (Cappellari+, 2011) J/MNRAS/414/888 : ATLAS3D project. III. (Emsellem+, 2011) J/MNRAS/414/940 : ATLAS3D project. IV. (Young+, 2011) Byte-by-byte Description of file: table2.dat table3.dat
Bytes Format Units Label Explanations
1- 10 A10 --- Gal Galaxy name 12- 16 F5.2 [Mpc-3] logRho10 Mean density of galaxies inside a sphere centred on the galaxy and containing the 10 nearest neighbours (1) 18- 22 F5.2 [Mpc-2] logSig10 Mean surface density of galaxies inside a cylinder of height h=600km/s (i.e. δVhel<300km/s) centred on the galaxy which contains the 10 nearest neighbours (2) 24- 28 F5.2 [Mpc-2] logSig3 Mean density of galaxies inside a sphere centred on the galaxy and containing the 3 nearest neighbours 30- 34 F5.2 [Lsun/Mpc3] logNu10 Mean K-band luminosity density of galaxies inside the sphere defined in logRho10 (3) 36- 40 F5.2 [Lsun/Mpc2] logI10 Mean K-band luminosity surface density of galaxies inside the cylinder defined in logSig10 42- 46 F5.2 [Lsun/Mpc2] logI3 Mean K-band luminosity surface density of galaxies inside the cylinder defined in logSig3
Note (1): All density estimators only include galaxies brighter than MK←21.5mag. Note (2): For galaxies in Virgo the cylinder includes all the cluster galaxies along the line of sight. Note (3): The galaxy luminosity is defined as LK=10^-0.4(MK-MK), where the solar absolute luminosity MK=3.29mag (Blanton & Roweis, 2007AJ....133..734B).
History: From electronic version of the journal References: Cappellari et al., Paper I 2011MNRAS.413..813C, Cat. J/MNRAS/413/813 Krajnovic et al., Paper II 2011MNRAS.414.2923K Emsellem et al., Paper III 2011MNRAS.414..888E, Cat. J/MNRAS/414/888 Young et al., Paper IV 2011MNRAS.414..940Y, Cat. J/MNRAS/414/940 Davis et al., Paper V 2011MNRAS.414..968D Bois et al., Paper VI 2011MNRAS.416.1654B Khochfar et al., Paper VIII 2011MNRAS.417..845K Duc et al., Paper IX 2011MNRAS.417..863D Davis et al., Paper X 2011MNRAS.417..882D Crocker et al., Paper XI 2012MNRAS.421.1298C
(End) Patricia Vannier [CDS] 26-Mar-2012
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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