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Cloud-scale ISM structure and star formation in M51

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We compare the structure of molecular gas at 40 pc resolution to the ability of gas to form stars across the disk of the spiral galaxy M51. We break the PAWS survey into 370 pc and 1.1 kpc resolution elements, and within each we estimate the molecular gas depletion time ( ##IMG## [http://ej.iop.org/...

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Main Authors: Leroy, Adam K. (Author) , Kruijssen, Diederik (Author) , Bigiel, Frank (Author) , Chevance, Mélanie (Author)
Format: Article (Journal)
Language:English
Published: 2017 August 31
In: The astrophysical journal
Year: 2017, Volume: 846, Issue: 1
ISSN:1538-4357
DOI:10.3847/1538-4357/aa7fef
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.3847/1538-4357/aa7fef
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Author Notes:Adam K. Leroy, Eva Schinnerer, Annie Hughes, J.M. Diederik Kruijssen, Sharon Meidt, Andreas Schruba, Jiayi Sun, Frank Bigiel, Gonzalo Aniano, Guillermo A. Blanc, Alberto Bolatto, Mélanie Chevance, Dario Colombo, Molly Gallagher, Santiago Garcia-Burillo, Carsten Kramer, Miguel Querejeta, Jerome Pety, Todd A. Thompson, and Antonio Usero
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Cloud scale ISM structure and star formation in M51 by Leroy, Adam K. (Author) , Kruijssen, Diederik (Author) , Bigiel, Frank (Author) , Chevance, Mélanie (Author) ,


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