The Star formation rate and dense molecular gas in galaxies - INSPIRE

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The Star formation rate and dense molecular gas in galaxies

Yu Gao
(
- Massachusetts U., Amherst and
- Caltech, IPAC
)
,
Philip M. Solomon
(
- SUNY, Stony Brook
)

Oct, 2003

20 pages

Published in:

Astrophys.J. 606 (2004) 271-290

e-Print:

astro-ph/0310339 [astro-ph]

DOI:

10.1086/382999

View in:

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Abstract: (arXiv)

(abridged) HCN luminosity Lhcn is a tracer of DENSE molecular gas, n(H_2) >~ 3x10^4 cm^{-3}, associated with star-forming giant molecular cloud (GMC) cores. We present the results and analysis of our survey of HCN emission from 65 infrared galaxies including 9 ultraluminous infrared galaxies (ULIGs, Lir>10^{12}Lsun), 22 luminous infrared galaxies (LIGs, 10^{11}

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Figures(0)

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