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Kennicutt-Schmidt relation in the HI dominated regime

Published online by Cambridge University Press:  09 February 2015

Sambit Roychowdhury
Affiliation:
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85748Garching, Germany email: sambit@mpa-garching.mpg.de
Mei-Ling Huang
Affiliation:
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85748Garching, Germany email: sambit@mpa-garching.mpg.de
Guinevere Kauffmann
Affiliation:
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85748Garching, Germany email: sambit@mpa-garching.mpg.de
Jayaram N. Chengalur
Affiliation:
NCRA-TIFR, Post Bag 3, Ganeshkhind, Pune411 007, India
Corresponding
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Abstract

We investigate the existence of a Kennicutt-Schmidt type relation between ΣSFR and Σgas, atomic in the HI dominated regions of nearby spirals and dwarf irregulars.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2015 

References

Begum, A., et al. 2008, MNRAS, 386, 1667CrossRefGoogle Scholar
Bigiel, F., et al. 2010, AJ, 140, 1194CrossRefGoogle Scholar
da Silva, R. L., Fumagalli, M., & Krumholz, M. R., 2014, arXiv:1403.4605Google Scholar
Hao, C.-N., et al. 2011, ApJ, 741, 124CrossRefGoogle Scholar
Kennicutt, R. C. Jr. 1998, ApJ, 498, 541CrossRefGoogle Scholar
Leroy, A. K., et al. 2013, AJ, 146, 19CrossRefGoogle Scholar
Roychowdhury, S., et al. 2014, MNRAS, in pressGoogle Scholar
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