Thermal feedback in the high-mass star- and cluster-forming region W51
High-mass stars have generally been assumed to accrete most of their mass while already contracted onto the main sequence, but this hypothesis has not been observationally tested. We present ALMA observations of a ##IMG## [http://ej.iop.org/images/0004-637X/842/2/92/apjaa6bfaieqn1.gif] $3\times 1.5$...
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| Main Authors: | , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
2017 June 16
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| In: |
The astrophysical journal
Year: 2017, Volume: 842, Issue: 2, Pages: 92 |
| ISSN: | 1538-4357 |
| DOI: | 10.3847/1538-4357/aa6bfa |
| Online Access: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.3847/1538-4357/aa6bfa
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| Author Notes: | Adam Ginsburg, Ciriaco Goddi, J.M. Diederik Kruijssen, John Bally, Rowan Smith, Roberto Galván-Madrid, Elisabeth A.C. Mills, Ke Wang, James E. Dale, Jeremy Darling, Erik Rosolowsky, Robert Loughnane, Leonardo Testi, and Nate Bastian |
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Thermal feedback in the high-mass star and cluster forming region W51
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