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The relationship between molecular gas, HI, and star formation in the low-mass, low-metallicity magellanic clouds

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The Magellanic Clouds provide the only laboratory to study the effects of metallicity and galaxy mass on molecular gas and star formation at high (∼⃒20 pc) resolution. We use the dust emission from HERITAGE Herschel data to map the molecular gas in the Magellanic Clouds, avoiding the known biases of...

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Main Authors: Jameson, Katherine E. (Author) , Bolatto, Alberto D. (Author) , Leroy, Adam K. (Author) , Meixner, Margaret (Author) , Roman-Duval, Julia (Author) , Gordon, Karl (Author) , Hughes, Annie (Author) , Israel, Frank P. (Author) , Rubio, Monica (Author) , Indebetouw, Remy (Author) , Madden, Suzanne C. (Author) , Bot, Caroline (Author) , Hony, Sacha (Author) , Cormier, Diane (Author) , Pellegrini, Eric W. (Author) , Galametz, Maud (Author) , Sonneborn, George (Author)
Format: Article (Journal)
Language:English
Published: 2016 June 27
In: The astrophysical journal
Year: 2016, Volume: 825, Issue: 1
ISSN:1538-4357
DOI:10.3847/0004-637X/825/1/12
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.3847/0004-637X/825/1/12
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Author Notes:Katherine E. Jameson, Alberto D. Bolatto, Adam K. Leroy, Margaret Meixner, Julia Roman-Duval, Karl Gordon, Annie Hughes, Frank P. Israel, Monica Rubio, Remy Indebetouw, Suzanne C. Madden, Caroline Bot, Sacha Hony, Diane Cormier, Eric W. Pellegrini, Maud Galametz, and George Sonneborn
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The relationship between molecular gas, HI, and star formation in the low-mass, low-metallicity magellanic clouds by Jameson, Katherine E. (Author) , Hony, Sacha (Author) , Cormier, Diane (Author) ,


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