Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
Scientific paper
2009-06-19
Astrophys.J.701:1398-1414,2009
Astronomy and Astrophysics
Astrophysics
Cosmology and Extragalactic Astrophysics
Final version as published, including minor corrections made in proof
Scientific paper
10.1088/0004-637X/701/2/1398
Star formation rates (SFR) are compared as determined from mid-infrared 7.7 um PAH luminosity [SFR(PAH)], from 1.4 GHz radio luminosity [SFR(radio)], and from far ultraviolet luminosity [SFR(UV)] for a sample of 287 starburst galaxies with z < 0.5 having Spitzer IRS observations. The previously adopted relation log [SFR(PAH)] = log [vLv(7.7 um)] - 42.57+-0.2, for SFR in solar masses per year and vLv(7.7 um) the luminosity at the peak of the 7.7 um PAH feature in ergs per s, is found to agree with SFR(radio). Comparing with SFR(UV) determined independently from ultraviolet observations of the same sources with the GALEX mission (not corrected for dust extinction), the median log [SFR(PAH)/SFR(UV)] = 1.67, indicating that only 2% of the ultraviolet continuum typically escapes extinction by dust within a starburst. The ratio SFR(PAH)/SFR(UV) depends on infrared luminosity, with form log [SFR(PAH)/SFR(UV)]= (0.53+-0.05)log Lir - 4.11+-0.18, for Lir in solar luminosities. We also find that the ratio SFR(PAH)/SFR(UV) is similar to that in infrared-selected starbursts for a sample of Markarian starburst galaxies originally selected using optical classification, which implies that there is no significant selection effect in SFR(PAH)/SFR(UV) using starburst galaxies discovered by Spitzer. These results indicate that SFRs determined with ultraviolet luminosities require dust corrections by a factor of ~ 10 for typical local starbursts but this factor increases to > 700 for the most luminous starbursts at z ~ 2.5. With this amount of extinction, the optical magnitude of a starburst having fv(7.7 um) of 1 mJy should be V ~ 25.6.
Sargsyan Lusine A.
Weedman Daniel W.
No associations
LandOfFree
Star Formation Rates for Starburst Galaxies from Ultraviolet, Infrared, and Radio Luminosities does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Star Formation Rates for Starburst Galaxies from Ultraviolet, Infrared, and Radio Luminosities, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Star Formation Rates for Starburst Galaxies from Ultraviolet, Infrared, and Radio Luminosities will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-401790