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1887
47604
The Relationship Between Molecular Gas, H I, and Star Formation in the Low-mass, Low-metallicity Magellanic Clouds
Author(s):
Jameson, K.E.; Bolatto, A.D.; Leroy, A.K.; Meixner, M.; Roman-Duval, J.; Gordon, K.; Hughes, A.; Israel, F.P.; Rubio, M.; Indebetouw, R.; Madden, S.C.; Bot, C.; Hony, S.; Cormier, D.; Pellegrini, EW.; Galametz, M.; Sonneborn, G.
Published
2016
Publication type
Article / Letter to editor
Date issued
2016
Language
English
Is part of
ASTROPHYSICAL JOURNAL (2016), Vol. 825, p. 12
hdl
1887/47604
doi
10.3847/0004-637X/825/1/12
URL
http://adsabs.harvard.edu/abs/2016ApJ...825...12J
Persistent identifier url
https://hdl.handle.net/1887/47604
Documents
01 - Astrophysical_Journal_825oe2016oe12
version: Not Applicable (or Unknown)
Full text at Publisher's site
Open Access