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2009-09-23
Does the LFIR-LHCN correlation hold for low LFIR isolated galaxies?
B. Ocana-FlaquerS. LeonD. EspadaS. Martin RuizU. LisenfeldS. VerleyJ. Sabater MontesL. Verdes-Montenegro
文献摘要
Low Isolated Galaxies (IGs) from the AMIGA sample have low level of Star Formation (SF) activity. We observed the HCN(1-0) emission in a sample of IGs in order to test whether they follow the tight relation between and found for galaxies with more active SF.
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