Schmidt–Kennicutt relations in SPH simulations of disc galaxies with effective thermal feedback from supernovae
Article first published online: 17 FEB 2012
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Monthly Notices of the Royal Astronomical Society
Volume 421, Issue 3, pages 2485–2497, April 2012
How to Cite
Monaco, P., Murante, G., Borgani, S. and Dolag, K. (2012), Schmidt–Kennicutt relations in SPH simulations of disc galaxies with effective thermal feedback from supernovae. Monthly Notices of the Royal Astronomical Society, 421: 2485–2497. doi: 10.1111/j.1365-2966.2012.20482.x
- Issue published online: 4 APR 2012
- Article first published online: 17 FEB 2012
- Accepted 2012 January 2. Received 2012 January 2; in original form 2011 February 14
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