A portrait of cold gas in galaxies at 60 pc resolution and a simple method to test hypotheses that link small-scale ISM structure to galaxy-scale processes
The cloud-scale density, velocity dispersion, and gravitational boundedness of the interstellar medium (ISM) vary within and among galaxies. In turbulent models, these properties play key roles in the ability of gas to form stars. New high-fidelity, high-resolution surveys offer the prospect to meas...
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2016 October 21
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| In: |
The astrophysical journal
Year: 2016, Jahrgang: 831, Heft: 1, Pages: 16 |
| ISSN: | 1538-4357 |
| DOI: | 10.3847/0004-637X/831/1/16 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.3847/0004-637X/831/1/16
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| Verfasserangaben: | Adam K. Leroy, Annie Hughes, Andreas Schruba, Erik Rosolowsky, Guillermo A. Blanc, Alberto D. Bolatto, Dario Colombo, Andres Escala, Carsten Kramer, J.M. Diederik Kruijssen, Sharon Meidt, Jerome Pety, Miguel Querejeta, Karin Sandstrom, Eva Schinnerer, Kazimierz Sliwa, and Antonio Usero |
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