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Disambiguation of "Kruijssen, J. M. Diederik"

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Physical Properties of Molecular Clouds at 2 parsec Resolution in the Low-Metallicity Dwarf Galaxy NGC 6822 and the Milky Way

, , , , , , , , and . (2017)cite arxiv:1701.02748Comment: Accepted for publication in The Astrophysical Journal; 22 pages, 10 figures, 7 tables.

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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 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).The implications of clustered star formation for (proto)planetary systems and habitability, and . (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 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.Formation versus destruction: the evolution of the star cluster population in galaxy mergers, , , , , and . (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 ALMA, , , , , , , , and . (2016)cite arxiv:1609.06316Comment: Accepted to ApJ, 18 pages, 15 figures.The dynamical state of stellar structure in star-forming regions, , , , , and . (2011)cite arxiv:1109.0986 Comment: 13 pages, 10 figures; Accepted for publication in MNRAS.The dynamical evolution of molecular clouds near the Galactic Centre -- III. Tidally--induced star formation in protocluster clouds, , and . (2019)cite arxiv:1903.10617Comment: 21 pages, 18 figures, accepted by MNRAS.Astro2020 Science White Paper: What is the lifecycle of gas and stars in galaxy centers?, , , , and . (2019)cite arxiv:1903.04525Comment: Submitted to the Astro2020 Decadal Survey.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, , , , , , , , , and 5 other author(s). (2020)cite arxiv:2001.07459Comment: Accepted for publication in ApJ, 32 pages, 11 figures.An uncertainty principle for star formation. I. Why galactic star formation relations break down below a certain spatial scale, and . (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/.