Magnetic Stability of Massive Star-forming Clumps in RCW 106
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/2041-8213/ab1346/pdf
Reference43 articles.
1. Interstellar Dust Grain Alignment
2. Molecular line mapping of the giant molecular cloud associated with RCW 106 - I. 13CO
3. THE THREE-MM ULTIMATE MOPRA MILKY WAY SURVEY. I. SURVEY OVERVIEW, INITIAL DATA RELEASES, AND FIRST RESULTS
4. Embedded Stellar Clusters in the W3/W4/W5 Molecular Cloud Complex
5. Magnetic Fields in Spiral Arms.
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1. High-mass Starless Clumps: Dynamical State and Correlation between Physical Parameters;The Astrophysical Journal;2023-05-25
2. 太赫兹混频器技术研究进展;Laser & Optoelectronics Progress;2023
3. The Role of Magnetic Fields in Triggered Star Formation of RCW 120;Research in Astronomy and Astrophysics;2022-06-22
4. H II regions and high-mass starless clump candidates;Astronomy & Astrophysics;2020-05
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