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Dense gas in the Galactic central molecular zone is warm and heated by turbulence

, , , , , , , , , , , , , , , , , , , , , and . (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.

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The signature of large scale turbulence driving on the structure of the interstellar medium, , , , , , , , , and 2 other author(s). (2022)cite arxiv:2206.00451Comment: 15 pages, 11 figures, to be published in MNRAS.What controls star formation in the central 500 pc of the Galaxy?, , , , , , and . (2013)cite arxiv:1303.6286Comment: 19 pages, 6 figures, 1 table, submitted to MNRAS.Constraints from Dust Mass and Mass Accretion Rate Measurements on Angular Momentum Transport in Protoplanetary Disks, , , , , , , and . (Aug 30, 2017)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.A deep learning approach for the 3D reconstruction of dust density and temperature in star-forming regions, , , , , , , , , and . (2023)cite arxiv:2308.09657Comment: 32 pages, 18 figures, submitted to Astronomy & Astrophysics, comments welcome.