Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-11-15
Astrophys.J.635:L173-L176,2005
Astronomy and Astrophysics
Astrophysics
10 pages, 2 figures. In press for ApJ Letters
Scientific paper
10.1086/499623
Observations have revealed prodigious amounts of star formation in starburst galaxies as traced by dust and molecular emission, even at large redshifts. Recent work shows that for both nearby spiral galaxies and distant starbursts, the global star formation rate, as indicated by the infrared luminosity, has a tight and almost linear correlation with the amount of dense gas as traced by the luminosity of HCN. Our surveys of Galactic dense cores in HCN 1-0 emission show that this correlation continues to a much smaller scale, with nearly the same ratio of infrared luminosity to HCN luminosity found over 7-8 orders of magnitude in L_IR, with a lower cutoff around 10^{4.5} L_sun of infrared luminosity. The linear correlation suggests that we may understand distant star formation in terms of the known properties of local star-forming regions. Both the correlation and the luminosity cutoff can be explained if the basic unit of star formation in galaxies is a dense core, similar to those studied in our Galaxy.
Evans II Neal. J.
Gao Yanfang
Shirley Yancy L.
Solomon Philip M.
Vanden Bout Paul A.
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