SPITZER 70 {mu}m EMISSION AS A STAR FORMATION RATE INDICATOR FOR SUB-GALACTIC REGIONS
Journal Article
·
· Astrophysical Journal
- Department of Astronomy, University of Massachusetts, Amherst, MA 01003 (United States)
- Institute of Astronomy, Cambridge University, Cambridge (United Kingdom)
- Steward Observatory, University of Arizona, AZ (United States)
- Department of Physics and Astronomy, University of Wyoming, WY (United States)
- Center for Astrophysics and Space Sciences, University of California, San Diego, CA (United States)
We use Spitzer 24 {mu}m, 70 {mu}m and ground-based H{alpha} data for a sample of 40 SINGS galaxies to establish a star formation rate (SFR) indicator using 70 {mu}m emission for sub-galactic ({approx}0.05-2 kpc) line-emitting regions and to investigate limits in application. A linear correlation between 70 {mu}m and SFR is found and a star formation indicator SFR(70) is proposed for line-emitting sub-galactic regions as {Sigma}(SFR)(M{sub sun} yr{sup -1} kpc{sup -2}) = 9.4 x 10{sup -44} {Sigma}(70)(erg s{sup -1} kpc{sup -2}), for regions with 12 + log(O/H) {approx}> 8.4 and {Sigma}(SFR) {approx}> 10{sup -3}(M{sub sun} yr{sup -1} kpc{sup -2}), with a 1{sigma} dispersion around the calibration of {approx}0.16 dex. We also discuss the influence of metallicity on the scatter of the data. Comparing with the SFR indicator at 70 {mu}m for integrated light from galaxies, we find that there is {approx}40% excess 70 {mu}m emission in galaxies, which can be attributed to stellar populations not involved in the current star formation activity.
- OSTI ID:
- 21474419
- Journal Information:
- Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 1 Vol. 725; ISSN ASJOAB; ISSN 0004-637X
- Country of Publication:
- United States
- Language:
- English
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