Hostname: page-component-8448b6f56d-cfpbc Total loading time: 0 Render date: 2024-04-19T19:22:56.111Z Has data issue: false hasContentIssue false

Star formation on galactic scales

Published online by Cambridge University Press:  01 August 2006

Robert C. Kennicutt Jr.*
Affiliation:
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK email: robk@ast.cam.ac.uk Steward Observatory, University of Arizona, Tucson, AZ 85721, USA
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

New multi-wavelength data on nearby galaxies are providing a much more accurate and complete observational picture of star formation on galactic scales. Here I briefly report on recent results from the Spitzer Infrared Nearby Galaxies Survey (SINGS). These provide new constraints on the frequency and lifetime of deeply obscured star-forming regions in galaxies, the measurement of dust-corrected star formation rates in galaxies, and the form of the spatially-resolved Schmidt law.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

References

Calzetti, D. et al. 2005, ApJ 633, 871CrossRefGoogle Scholar
Dale, D.A. et al. 2005, ApJ 633, 857Google Scholar
Gordon, K.D., Clayton, G.C., Witt, A.N. & Misselt, K.A. 2000, ApJ 602, 723Google Scholar
Helfer, T.T. et al. 2003, ApJS 145, 259CrossRefGoogle Scholar
Heyer, M.H., Corbelli, E., Schneider, S.E. & Young, J.S. 2004, ApJ 533, 236Google Scholar
Kennicutt, R.C. 2003, PASP 115, 98CrossRefGoogle Scholar
Kennicutt, R.C. 1998a, ARA&A 36,189Google Scholar
Kennicutt, R.C. 1998b, ApJ 498, 541CrossRefGoogle Scholar
Moustakas, J. & Kennicutt, R.C. 2006, ApJS 164, 81CrossRefGoogle Scholar
Pérez-Gonzaĺez, et al. 2006, ApJ 648, 987Google Scholar