Constraints on the Evolution of Luminous Compact Blue Galaxies from HI Observations

Astronomy and Astrophysics – Astronomy

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Scientific paper

Luminous Compact Blue Galaxies (LCBGs) are common at z 1, contributing 40% of the total star formation rate density athig that time, but are a factor of ten rarer by the present day. While we know that LCBGs are rapidly evolving, we do not know what drives their evolution or into what type of galaxy they evolve. We present original and archival HI data from Arecibo, the Green Bank Telescope (GBT), Nancay, and Parkes for a sample of local analogs to the intermediate redshift LCBGs. These data provide us with a measure of the fuel for future star formation and the dynamical masses of LCBGs; information that we can not currently obtain for z 1 LCBGs. The data reveal that LCBGs are a diverse collection of galaxies. LCBGs are gas-rich and prolifically forming stars, such that the majority will consume their HI within 5 Gyr. LCBGs have dynamical masses consistent with low-mass galaxies, such as dwarf ellipticals, dwarf irregular or late-type spirals. If intermediate redshift LCBGs have similar physical properties to their local counterparts, then it is unlikely that they will evolve into today's population of massive ellipticals and grand-design spirals nor into dwarf spheroidal galaxies.

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