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A model for the onset of self-gravitation and star formation in molecular gas governed by galactic forces: II. the bottleneck to collapse set by cloud-environment decoupling

S. Meidt, S. Glover, J. Kruijssen, A. Leroy, E. Rosolowsky, A. Schruba, A. Hughes, E. Schinnerer, A. Usero, F. Bigiel, G. Blanc, M. Chevance, J. Pety, M. Querejeta, and D. Utomo. (2020)cite arxiv:2001.07459Comment: Accepted for publication in ApJ, 32 pages, 11 figures.

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J J M Ramakers

J M Zöllner

Diederik Noordveld

J A M Wanders

Gabriele J M Demetz

Other publications of authors with the same name

The JWST Galactic Center Survey -- A White PaperR. Schoedel, S. Longmore, J. Henshaw, A. Ginsburg, J. Bally, A. Feldmeier, M. Hosek, F. Lara, A. Ciurlo, M. Chevance 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).The implications of clustered star formation for (proto)planetary systems and habitabilityJ. Kruijssen, and S. Longmore. (2019)cite arxiv:1901.04491Comment: 5 pages, 1 figure; to appear in the proceedings of IAU Symposium 345, Origins: from the Protosun to the First Steps of Life, Eds. B. G. Elmegreen, L. V. Tóth, M. Güdel, Cambridge University Press.Dense gas in the Galactic central molecular zone is warm and heated by turbulenceA. Ginsburg, C. Henkel, Y. Ao, D. Riquelme, J. Kauffmann, T. Pillai, E. Mills, M. Requena-Torres, K. Immer, L. Testi 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 dynamical state of stellar structure in star-forming regionsJ. Kruijssen, T. Maschberger, N. Moeckel, C. Clarke, N. Bastian, and I. Bonnell. (2011)cite arxiv:1109.0986 Comment: 13 pages, 10 figures; Accepted for publication in MNRAS.Formation versus destruction: the evolution of the star cluster population in galaxy mergersJ. Kruijssen, F. Pelupessy, H. Lamers, S. Zwart, N. Bastian, and V. Icke. (2011)cite arxiv:1112.1065Comment: 15 pages, 9 figures, 2 tables; Accepted for publication in MNRAS. A movie of the full time sequence in Figure 1 can be found at http://www.mpa-garching.mpg.de/~diederik/1m11clusters.html.The Molecular Wind in the Nearest Seyfert Galaxy Circinus Revealed by ALMAL. Zschaechner, F. Walter, A. Bolatto, E. Farina, J. Kruijssen, A. Leroy, D. Meier, J. Ott, and S. Veilleux. (2016)cite arxiv:1609.06316Comment: Accepted to ApJ, 18 pages, 15 figures.The dynamical evolution of molecular clouds near the Galactic Centre -- III. Tidally--induced star formation in protocluster cloudsJ. Dale, J. Kruijssen, and S. Longmore. (2019)cite arxiv:1903.10617Comment: 21 pages, 18 figures, accepted by MNRAS.An uncertainty principle for star formation. I. Why galactic star formation relations break down below a certain spatial scaleJ. Kruijssen, and S. Longmore. (2014)cite arxiv:1401.4459Comment: 14 pages (including appendices), 5 figures, 2 tables; accepted by MNRAS (15 January 2014). Fortran and IDL routines for applying the uncertainty principle are publicly available at http://www.mpa-garching.mpg.de/KL14principle/.What controls star formation in the central 500 pc of the Galaxy?J. Kruijssen, S. Longmore, B. Elmegreen, N. Murray, J. Bally, L. Testi, and R. Kennicutt Jr.. (2013)cite arxiv:1303.6286Comment: 19 pages, 6 figures, 1 table, submitted to MNRAS.Physical Properties of Molecular Clouds at 2 parsec Resolution in the Low-Metallicity Dwarf Galaxy NGC 6822 and the Milky WayA. Schruba, A. Leroy, J. Kruijssen, F. Bigiel, A. Bolatto, W. de Blok, L. Tacconi, E. van Dishoeck, and F. Walter. (2017)cite arxiv:1701.02748Comment: Accepted for publication in The Astrophysical Journal; 22 pages, 10 figures, 7 tables.

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