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 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:
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FileName Lrecl Records Explanations
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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
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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)
J/MNRAS/433/2812 : ATLAS3D project. XXIII (Krajnovic+, 2013)
J/MNRAS/446/120 : ATLAS3D project. XXIX (Duc+, 2015)
J/MNRAS/448/3484 : ATLAS3D Project. XXX (McDermid+, 2015)
Byte-by-byte Description of file: table2.dat table3.dat
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Bytes Format Units Label Explanations
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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
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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 2007AJ....133..734B).
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History:
From electronic version of the journal
References:
Cappellari et al., Paper I 2011MNRAS.413..813C 2011MNRAS.413..813C, Cat. J/MNRAS/413/813
Krajnovic et al., Paper II 2011MNRAS.414.2923K 2011MNRAS.414.2923K
Emsellem et al., Paper III 2011MNRAS.414..888E 2011MNRAS.414..888E, Cat. J/MNRAS/414/888
Young et al., Paper IV 2011MNRAS.414..940Y 2011MNRAS.414..940Y, Cat. J/MNRAS/414/940
Davis et al., Paper V 2011MNRAS.414..968D 2011MNRAS.414..968D
Bois et al., Paper VI 2011MNRAS.416.1654B 2011MNRAS.416.1654B
Khochfar et al., Paper VIII 2011MNRAS.417..845K 2011MNRAS.417..845K
Duc et al., Paper IX 2011MNRAS.417..863D 2011MNRAS.417..863D
Davis et al., Paper X 2011MNRAS.417..882D 2011MNRAS.417..882D
Crocker et al., Paper XI 2012MNRAS.421.1298C 2012MNRAS.421.1298C
Lablanche et al., Paper XII 2012MNRAS.424.1495L 2012MNRAS.424.1495L
Serra et al., Paper XIII 2012MNRAS.422.1835S 2012MNRAS.422.1835S
Krajnovic et al., Paper XIV 2013MNRAS.432.1768K 2013MNRAS.432.1768K
Cappellari et al., Paper XV 2013MNRAS.432.1709C 2013MNRAS.432.1709C
Bayet et al., Paper XVI 2013MNRAS.432.1742B 2013MNRAS.432.1742B
Krajnovic et al., Paper XVII 2013MNRAS.432.1768K 2013MNRAS.432.1768K
Alatalo et al., Paper XVIII 2013MNRAS.432.1796A 2013MNRAS.432.1796A
Sarzi et al., Paper XIX 2013MNRAS.432.1845S 2013MNRAS.432.1845S
Cappellari et al., Paper XX 2013MNRAS.432.1862C 2013MNRAS.432.1862C
Scott et al., Paper XXI 2013MNRAS.432.1894S 2013MNRAS.432.1894S
Martig et al., Paper XXII 2013MNRAS.432.1914M 2013MNRAS.432.1914M
Krajnovic et al., Paper XXIII 2013MNRAS.433.2812K 2013MNRAS.433.2812K, Cat. J/MNRAS/433/2812
Davis et al., Paper XXIV 2013MNRAS.429..534D 2013MNRAS.429..534D
Cappellari et al., Paper XXV 2013MNRAS.432.1709C 2013MNRAS.432.1709C
Bayet et al., Paper XXVI 2013MNRAS.432.1742B 2013MNRAS.432.1742B
Krajnovic et al., Paper XXVII 2013MNRAS.432.1768K 2013MNRAS.432.1768K
Alatalo et al., Paper XXVIII 2013MNRAS.432.1796A 2013MNRAS.432.1796A
Duc et al., Paper XXIX 2015MNRAS.446..120D 2015MNRAS.446..120D
McDermid et al., Paper XXX 2015MNRAS.448.3484M 2015MNRAS.448.3484M, Cat. J/MNRAS/448/3484
(End) Patricia Vannier [CDS] 26-Mar-2012