Mapping the properties of blue compact dwarf galaxies: integral field spectroscopy with PMAS

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Table 1:

The galaxy sample.
Galaxy	RA	Dec	$m_{\rm B}$	D	$M_{\rm B}$	$A_{\rm B}$
	(J2000)	(J2000)		(Mpc)	(mag)	(mag)
Mrk 407	09 47 47.6	+39 05 04	$15.39\pm0.49$	27.2	-16.78	0.069
Mrk 32	10 27 02.0	+56 16 14	$16.08\pm0.11$	16.4	-14.99	0.030
Mrk 750	11 50 02.7	+15 01 24	$15.76\pm0.54$	05.2	-12.82	0.175
Mrk 206	12 24 17.0	+67 26 24	$15.40\pm0.07$	24.3	-16.53	0.071
Tololo 1434+032	14 37 08.9	+03 02 50	$16.91\pm0.86$	29.2	-15.42	0.149
Mrk 475	14 39 05.4	+36 48 22	$16.41\pm0.31$	11.9	-13.97	0.052
I Zw 123	15 37 04.2	+55 15 48	$15.44\pm0.08$	15.4	-15.50	0.062
I Zw 159	16 35 21.0	+52 12 53	$15.65\pm0.28$	43.8	-17.56	0.125

Notes. RA, Dec, D and $A_{\rm B}$ taken from the NED (http://nedwww.ipac.caltech.edu/). Distances were computed using a Hubble constant of 73 km s^-1 Mpc^-1 and taking into account the influence of the Virgo Cluster, the Great Attractor and the Shapley supercluster. $m_{\rm B}$ taken from HyperLeda (http://leda.univ-lyon1.fr/; Paturel et al. 2003) and $M_{\rm B}$ computed from the tabulated values of $m_{\rm B}$ and D.

Source LaTeX | All tables | In the text

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