The host in blue compact galaxies. - Structural properties and scaling relations

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Volume 501 / No 1 (July I 2009)

A&A, 501 1 (2009) 75-88

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Table 3:

HI gas and stellar properties for the analysed galaxies.
Galaxy	$W^{\rm c}_{\rm 20}$	$M_{\rm HI}$	M_s/L_B	$M_{\rm s}$	$M_{\rm HI}/L_{B}$
	[km s^-1]	[10⁹ $M_{\odot}$ ]	[ $M_{\odot}$ $/L_{\odot}$ ]	[10⁹ $M_{\odot}$ ]	[ $M_{\odot}$ $/L_{\odot}$ ]
(1)	(2)	(3)	(4)	(5)	(6)
Mrk 5	90	0.14	0.41	0.07	0.86
Mrk 33	196	0.54	2.19	3.55	0.34
Mrk 35	135	0.68	1.15	0.98	0.80
Mrk 36	78	0.03	0.85	0.03	0.87
Mrk 86	87	0.32	2.40	1.75	0.44
Mrk 314	269	2.51	0.09	0.21	1.11
Mrk 324	135	0.23	1.37	0.50	0.67
Mrk 370	187	0.29	1.12	0.83	0.40
Mrk 401	148	0.82	0.38	0.57	0.55
Mrk 600	102	0.24	0.28	0.05	1.22
PHL 293 B	124	0.20	0.47	0.03	3.41
I Zw 123	105	0.06	1.25	0.12	0.68
II Zw 70	123	0.43	0.45	0.10	1.84
II Zw 71	180	0.95	1.00	0.65	1.41
III Zw 102	183	1.98	1.94	7.88	0.49

Notes: Cols.: (2) Hydrogen line width at 20% after inclination and random motion corrections (see Sect. 5.2). (3) HI mass after correcting from differences in galaxy distances (see text). The original quantities of (2) and (3) were taken from Thuan & Martin (1981) excepting Mrk 36, Mrk 324, Mrk 370 and III Zw 102 for which line width data was taken from Springob et al. (2005). (4) Mass-luminosity relation derived for the BCG hosts (see Sect. 5.2); (5) Stellar mass, estimated from the host absolute magnitudes (see Table 4) and the M/L values listed in (4); (6) HI gas mass-to-B-band host luminosity ratio.

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