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arXiv · 0909.4192

Does the LFIR-LHCN correlation hold for low LFIR isolated galaxies?

B. Ocana-Flaquer·S. Leon·D. Espada·S. Martin Ruiz·U. Lisenfeld·S. Verley·J. Sabater Montes·L. Verdes-Montenegro
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Abstract

Low $L_{FIR}$ 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 $L_{HCN}$ and $L_{FIR}$ found for galaxies with more active SF.

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B. Ocana-Flaquer, S. Leon, D. Espada, S. Martin Ruiz, U. Lisenfeld, S. Verley, J. Sabater Montes, L. Verdes-Montenegro. 2009-09-23. Does the LFIR-LHCN correlation hold for low LFIR isolated galaxies?. https://arxiv.org/abs/0909.4192

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