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Low Virial Parameters in Molecular Clouds: Implications for High Mass Star Formation and Magnetic Fields

, , and . (2013)cite arxiv:1308.5679Comment: accepted to ApJ.

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Low Virial Parameters in Molecular Clouds: Implications for High Mass Star Formation and Magnetic Fields, , and . (2013)cite arxiv:1308.5679Comment: accepted to ApJ.Dense gas in the Galactic central molecular zone is warm and heated by turbulence, , , , , , , , , and 12 other author(s). (2015)cite arxiv:1509.01583Comment: Accepted to A&A. The data (raw & processed) are available from http://doi.org/10.7910/DVN/27601 . The processing pipeline, analysis code, and paper source are available at https://github.com/adamginsburg/APEX_CMZ_H2CO.The JWST Galactic Center Survey -- A White Paper, , , , , , , , , and 81 other author(s). (2023)cite arxiv:2310.11912Comment: This White Paper will be updated when required (e.g. new authors joining, editing of content).LivOlay: interactive ad-hoc registration and overlapping of applications for collaborative visual exploration., , , , , and . CHI, page 1357-1360. ACM, (2008)A Simple Perspective on the Mass-Area Relationship in Molecular Clouds, , , , , , and . (2012)cite arxiv:1204.2557Comment: 10 pages, 8 figures, MNRAS in press.