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Dwarf galaxies in the nearby Lynx-Cancer void: photometry, colours and ages

The nearby Lynx-Cancer void is a good laboratory to study the effect of very rarefied environment on the evolution of the least massive dwarf galaxies. A recently compiled sample of this void's galaxies includes about one hundred objects with M_B in the range -12 to -18 mag. Good quality images are available in the SDSS database for ~80% of the sample. Their u,g,r,i,z photometry allows one to derive galaxy stellar mass (and, incorporating HI data, gas mass-fraction) and ages of visible stellar populations, and hence, the epoch of their formation (first SF episode). We present the first photometric results of the ongoing study of the Lynx-Cancer void.

preprint2010arXivOpen access
S. PustilnikA. KniazevY. LyaminaA. Tepliakova
astro-ph.COastro-ph.GA
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S. PustilnikA. KniazevY. LyaminaA. Tepliakova

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