The relationship between molecular gas, HI, and star formation in the low-mass, low-metallicity magellanic clouds
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...
Gespeichert in:
| Hauptverfasser: | , , , , , , , , , , , , , , , , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2016 June 27
|
| In: |
The astrophysical journal
Year: 2016, Jahrgang: 825, Heft: 1 |
| ISSN: | 1538-4357 |
| DOI: | 10.3847/0004-637X/825/1/12 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.3847/0004-637X/825/1/12
|
| Verfasserangaben: | 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 |
Search Result 1
The relationship between molecular gas, HI, and star formation in the low-mass, low-metallicity magellanic clouds
Article (Journal)
Kapitel/Artikel
Online Resource