Molecular Cloud Cores in the Galactic Center 50 km s−1 Molecular Cloud
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/872/i=2/a=121/pdf
Reference47 articles.
1. Mapping photodissociation and shocks in the vicinity of Sagittarius A∗
2. From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from theHerschelGould Belt Survey
3. The thermal state of molecular clouds in the Galactic center: evidence for non-photon-driven heating
4. Star formation rates and efficiencies in the Galactic Centre
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1. A Broad Line-width, Compact, Millimeter-bright Molecular Emission Line Source near the Galactic Center;The Astrophysical Journal Letters;2024-06-01
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3. The episodic and multiscale Galactic Centre;New Astronomy Reviews;2021-12
4. Dynamically Driven Inflow onto the Galactic Center and its Effect upon Molecular Clouds;The Astrophysical Journal;2021-11-01
5. Hot molecular core candidates in the Galactic center 50 km s−1 molecular cloud;Publications of the Astronomical Society of Japan;2021-06-22
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