arXiv · 1011.3422
Metallicities of galaxies in the nearby Lynx-Cancer void
Abstract
Does the void environment have a sizable effect on the evolution of dwarf galaxies? If yes, the best probes should be the most fragile least massive dwarfs. We compiled a sample of about one hundred dwarfs with M_B in the range -12 to -18 mag, falling within the nearby Lynx-Cancer void. The goal is to study their evolutionary parameters -- gas metallicity and gas mass-fraction, and to address the epoch of the first substantial episode of Star Formation. Here we present and discuss the results of O/H measurements in 38 void galaxies, among which several the most metal-poor galaxies are found with the oxygen abundances of 12+log(O/H)=7.12-7.3 dex.
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A. Kniazev, S. Pustilnik, A. Tepliakova, A. Burenkov. 2010-11-15. Metallicities of galaxies in the nearby Lynx-Cancer void. https://doi.org/10.1007/978-3-642-20285-8_4
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