GALEX UV properties of the polar ring galaxy MCG-05-07-001 and the shell galaxies NGC 1210 and NGC 5329

A. Marino; E. Iodice; R. Tantalo; L. Piovan; D. Bettoni; L. M. Buson; C. Chiosi; G. Galletta; R. Rampazzo; R. M. Rich

doi:10.1051/0004-6361/200911819

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Volume 508 / No 3 (December IV 2009)

A&A, 508 3 (2009) 1235-1252

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Table 6:

Relevant properties of the adopted chemical and dusty model for the simulated galaxy.
The basic chemical model
Total mass of galaxy $M_{\rm tot}$	$1.30\times 10^{10}~M_{\odot}$
Total mass of gas $M_{\rm gas}$	$7.82\times 10^{9}~M_{\odot}$
Total mass of stars $M_{\rm tot}$	$5.06\times 10^{9}~M_{\odot}$
Fraction of gas $M_{\rm gas}/M_{\rm tot}$	0.6
Metallicity Z	0.0178
Time of galactic wind^a	1.09 Gyr
The associated EPS model with dust
Total radius	15 Kpc
Fraction of molecular gas $M_{\rm mol}/M_{\rm gas}$	0.3
Evaporation time of MCs^b	30 Myr

^a Duration of the SFH; ^b time scale needed to evaporate the MC in which a new generation of stars is embedded.

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