Kennicutt-Schmidt Law in the Central Region of NGC 4321 as Seen by ALMA
Author:
Publisher
Springer Science and Business Media LLC
Subject
Multidisciplinary
Link
http://www.nature.com/articles/srep26896.pdf
Reference47 articles.
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3. Schmidt, M. The rate of star formation. Astrophys. J. 129, 243–258 (1959).
4. Wong, T. & Blitz, L. The relationship between gas content and star formation in molecule-rich spiral galaxies. Astrophys. J. 569, 157–183 (2002).
5. Momose, R. et al. Star formation on subkiloparsec scale triggered by non-linear processes in nearby spiral galaxies. Astrophys. J. 772, L13–L17 (2013).
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