The diverse X-ray properties of four truly isolated elliptical galaxies: NGC 2954, NGC 6172, NGC 7052, and NGC 7785

E. Memola; G. Trinchieri; A. Wolter; P. Focardi; B. Kelm

doi:10.1051/0004-6361/200810801

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Volume 497 / No 2 (April II 2009)

A&A, 497 2 (2009) 359-370

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Table 1:

Basic optical parameters for the isolated galaxies. Galaxy distances are Virgo-centric.
Source	Vel.	D	Scale	Opt $_{\rm dim}$	Log L_B	Log L_K	Log M_*
	km s^-1	Mpc	kpc/ $\hbox {$^{\prime \prime }$ }$	$\hbox{$^\prime$ }$	$L_{B_\odot}$	$L_{K_\odot}$	$M_\odot$
NGC 2954	3774	51	0.241	$1.1\times1.7$	10.36	11.00	10.78
NGC 6172	5085	69	0.323	$1.0\times1.0$	10.46	11.12	10.92
NGC 7052	5082	69	0.323	$1.4\times2.5$	10.61	11.61	11.41
NGC 7785	3876	52	0.247	$1.3\times2.5$	10.70	11.42	11.22

Source LaTeX | All tables | In the text

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