Study of gravitational fields and globular cluster systems of early-type galaxies

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Volume 625 (May 2019)

A&A, 625 (2019) A32

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Table 1.

Galaxy sample.

Name	d	1′	log L	R_e	n	B − V	Type	Env	Prof	Iso	λ_{R_e}	ϵ	Rot
	(Mpc)	(kpc)	(L_⊙)	(kpc)		(mag)
N 821	24	7.0	10.5	4.7 ⁽¹⁴⁾	4.7 ⁽¹⁴⁾	0.87	E6 ⁽¹⁹⁾	F ⁽¹⁹⁾	∣ ⁽¹⁾	D ^(7, 9)	0.27 ⁽⁸⁾	0.35 ⁽⁸⁾	f
N 1023	11.4	3.3	10.5	2.7 ⁽²⁸⁾	4.2 ⁽²⁸⁾	0.91	S0 ⁽⁸⁾	G ⁽²⁸⁾	\ ⁽¹⁾	D ⁽⁵⁾	0.39 ⁽⁸⁾	0.63 ⁽⁸⁾	f
N 1399	20	5.8	10.7	3.5 ⁽¹⁵⁾	5.6 ⁽¹⁵⁾	0.93	E1pec ⁽²⁴⁾	C ⁽²⁴⁾	∩ ⁽¹⁾	D ⁽¹⁰⁾	0.08 ⁽¹¹⁾	0.09 ⁽¹¹⁾	s
N 1400	26	7.7	10.4	3.4 ⁽¹⁴⁾	4.0 ⁽¹⁴⁾	0.89	S0/E0 ⁽¹⁹⁾	G ⁽¹⁹⁾	∩ ⁽¹⁾	0 ⁽²⁾	0.27 ⁽⁸⁾	0.11 ⁽⁸⁾	f
N 1407	29	8.4	11.0	9.4 ⁽¹⁴⁾	8.3 ⁽¹⁴⁾	0.95	E0 ⁽¹⁹⁾	G ⁽¹⁹⁾	∩⁽²⁾	0 ⁽²⁾	0.08 ⁽⁸⁾	0.05 ⁽⁸⁾	f
N 2768	22	6.5	10.7	8.9 ⁽¹⁶⁾	3.3 ⁽¹⁶⁾	0.91	E6/S0	G ⁽¹⁹⁾	? ⁽³⁾	D ⁽⁵⁾	0.25 ⁽⁸⁾	0.57 ⁽⁸⁾	f
N 3115	9.7	2.8	10.2	4.8 ⁽¹⁷⁾	4.4 ⁽¹⁷⁾	0.90	S0 ⁽¹⁹⁾	F ⁽¹⁹⁾	\ ⁽¹⁾	D ⁽⁶⁾	0.58 ⁽⁸⁾	0.49 ⁽⁸⁾	f
N 3377	11.2	3.3	9.9	2.9 ⁽¹⁶⁾	5.0 ⁽¹⁶⁾	0.82	E6 ⁽¹⁹⁾	G ⁽¹⁹⁾	\ ⁽¹⁾	D ⁽⁵⁾	0.52 ⁽⁸⁾	0.33 ⁽⁸⁾	f
N 4278	16	4.7	10.2	2.5 ⁽¹⁶⁾	4.8 ⁽¹⁶⁾	0.90	E1-2 ⁽¹⁹⁾	G ⁽¹⁹⁾	∩ ⁽¹⁾	B ⁽⁵⁾	0.18 ⁽⁸⁾	0.09 ⁽⁸⁾	f
N 4365	20	5.9	10.7	8.5 ⁽¹⁸⁾	5.2 ⁽¹⁸⁾	0.93	E3 ⁽¹⁹⁾	G ⁽¹⁹⁾	∩ ⁽¹⁾	B ⁽⁷⁾	0.09 ⁽⁸⁾	0.24 ⁽⁸⁾	s
N 4472	16.3	4.7	10.9	3.9 ⁽¹⁵⁾	3.0 ⁽¹⁵⁾	0.93	E2 ⁽²⁴⁾	C ⁽²⁴⁾	∩ ⁽¹⁾	B ^(7, 9)	0.077 ⁽⁹⁾	0.172 ⁽⁹⁾	s
N 4486	16	4.7	10.8	5.8 ⁽¹⁸⁾	2.9 ⁽¹⁸⁾	0.92	E0 ⁽¹⁹⁾	C ⁽¹⁹⁾	∩ ⁽¹⁾	B ⁽⁵⁾	0.02 ⁽⁸⁾	0.16 ⁽⁸⁾	s
N 4494	17.1	5.0	10.4	3.7 ⁽¹⁶⁾	3.4 ⁽¹⁶⁾	0.85	E1-E2 ⁽¹⁹⁾	G ⁽¹⁹⁾	\ ⁽¹⁾	D ⁽⁷⁾	0.21 ⁽⁸⁾	0.14 ⁽⁸⁾	f
N 4526	17	4.9	10.4	2.7 ⁽²⁸⁾	3.6 ⁽²⁸⁾	0.89	S0 ⁽⁸⁾	C ⁽²⁸⁾	?	B ⁽⁵⁾	0.45 ⁽⁸⁾	0.76 ⁽⁸⁾	f
N 4649	17	4.9	10.8	5.1 ⁽¹⁵⁾	3.6 ⁽¹⁵⁾	0.93	E2/S0 ⁽⁸⁾	C ⁽²⁴⁾	∩ ⁽¹⁾	B ^(7, 9)	0.127 ⁽⁹⁾	0.156 ⁽⁹⁾	f
N 5128	4.2	1.2	10.5	6.2 ⁽¹⁴⁾	4.0 ⁽¹⁴⁾	0.87	S0pec/Epec ⁽²⁵⁾	G ⁽²⁶⁾	? ⁽¹²⁾	? ⁽¹³⁾	0.15 ⁽¹³⁾	0.05 ⁽²⁷⁾	f
N 5846	25	7.2	10.7	8.1 ⁽¹⁶⁾	3.9 ⁽¹⁶⁾	0.94	E0 ⁽¹⁹⁾	G ⁽¹⁹⁾	? ⁽⁴⁾	B ⁽⁵⁾	0.03 ⁽⁸⁾	0.08 ⁽⁸⁾	s

R17x	19	5.5	10.2	1.5	2.6	0.90	–	–		–	–	–	–
R17y	19	5.5	10.2	1.7	2.0	0.90	–	–		–	–	–	–
R17z	19	5.5	10.2	2.0	2.0	0.90	–	–		–	–	–	–

Notes. d – Galaxy distance and its uncertainties according to Tonry et al. (2001). 1′ – The distance corresponding to 1′ if the galaxy is found at the distance of d. L – Galaxy B-band luminosity calculated from d and the apparent magnitude listed in the HyperLeda database (http://leda.univ-lyon1.fr/) (Makarov et al. 2014). R_e – Sérsic effective radius the galaxy according to the cited works assuming the galaxy distance d. n – Sérsic index of the galaxy. B – V – Color index according to the HyperLeda database. Type – Galaxy morphological type. Env – Galaxy environment (F = field, G = group, C = cluster). Prof – Galaxy central photometric profile (∩ is core, \ is power law, ∣ is intermediate, and “?” is unknown). Iso – Isophotal shape (“D” indicates disky isophotes, “B” indicates boxy isophotes, “0” indicates pure ellipses, and “?” indicates unknown because of observational problems). λ_{R_e} – Degree of rotational support of the galaxy (Eq. (24)). For NGC 5128, λ_{R_e} was estimated from Fig. 14 in Coccato et al. (2009) as an approximate average between the last measured data point for the stellar kinematics and from the planetary nebula kinematics at 1 R_e. ϵ – Galaxy ellipticity. Rot – Galaxy rotator type (“s” indicates slow and “f” indicates fast rotators) as determined using the rotator criterion number.

References. (1) Lauer et al. (2007); (2) Spolaor et al. (2008); (3) Lauer et al. (2005); (4) Rest et al. (2001); (5) Emsellem et al. (2007); (6) Nieto et al. (1991); (7) Bender et al. (1989); (8) Arnold et al. (2014); (9) Emsellem et al. (2011); (10) Kissler-Patig et al. (1997); (11) Scott et al. (2014); (12) Israel (1998); (13) Coccato et al. (2009); (14) Saxton & Ferreras (2010); (15) Dullo & Graham (2014); (16) Krajnović et al. (2013); (17) Hu (2008); (18) Kormendy et al. (2009); (19) Pota et al. (2013); (24) NASA Extragalactic Database (https://ned.ipac.caltech.edu/); (25) Harris (2010); (26) De Vaucouleurs et al. (1975); (27) Cappellari et al. (2009); (28) Alabi et al. (2017).

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