HCN J = 4–3, HNC J = 1–0, H13CN J = 1–0, and HC3N J = 10–9 Maps of Galactic Center Region. II. Physical Properties of Dense-gas Clumps and Probability of Star Formation-Reference-Cited by-同舟云学术

HCN J = 4–3, HNC J = 1–0, H13CN J = 1–0, and HC3N J = 10–9 Maps of Galactic Center Region. II. Physical Properties of Dense-gas Clumps and Probability of Star Formation

Published:2020-11-09 Issue:2 Volume:903 Page:111
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Tanaka Kunihiko^ORCID,Nagai Makoto,Kamegai Kazuhisa^ORCID,Iino Takahiro^ORCID,Sakai Takeshi^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/abbcca/pdf

Reference78 articles.

1. The thermal state of molecular clouds in the Galactic center: evidence for non-photon-driven heating

2. A multi-line ammonia survey of the Galactic center region with the Tsukuba 32 m telescope. I. Observations and data

3. Star formation rates and efficiencies in the Galactic Centre

4. Pressure-confined clumps in magnetized molecular clouds

5. Understanding the kinematics of Galactic Centre gas

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