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Disambiguation of "Ott, Juergen"

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Tracing Cold HI Gas in Nearby, Low-Mass Galaxies

, , , , , , , , and . (2012)cite arxiv:1208.0983Comment: 44 pages, 13 figures, Accepted for publication in ApJ.

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Juergen Runge

Juergen Kiener

Juergen Kroymann

Juergen Roemer

Juergen Seitz

 

Other publications of authors with the same name

VLA-ANGST: A high-resolution HI Survey of Nearby Dwarf Galaxies, , , , , , , , and . (2012)cite arxiv:1208.3737Comment: 64 figures, grouped into 32. 115 pages, accepted for publication in the Astronomical Journal.Tracing Cold HI Gas in Nearby, Low-Mass Galaxies, , , , , , , , and . (2012)cite arxiv:1208.0983Comment: 44 pages, 13 figures, Accepted for publication in ApJ.The Formation of Kiloparsec-Scale HI Holes in Dwarf Galaxies, , , , , , , , , and 4 other author(s). (2011)cite arxiv:1105.4117 Comment: 49 pages, 18 figures. Accepted for publication in ApJ.The Multi-Phase Cold Fountain in M82 Revealed by a Wide, Sensitive Map of the Molecular ISM, , , , , , , , , and . (2015)cite arxiv:1509.02932Comment: 36 pages including 25 figures and 4 appendices. Accepted for publication in the Astrophysical Journal. For a high resolution version please visit http://www.astronomy.ohio-state.edu/~leroy.42/ms_m82.pdf.Distance Determinations to SHIELD Galaxies from HST Imaging, , , , , , , , , and 2 other author(s). (2014)cite arxiv:1402.3723Comment: 15 pages, 6 figures, 2 tables.The Survey of HI in Extremely Low-mass Dwarfs (SHIELD), , , , , , , , , and 7 other author(s). (2011)cite arxiv:1105.4505 Comment: Accepted for publication in the Astrophysical Journal Letters EVLA Special Edition.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.Characterizing the transition from diffuse atomic to dense molecular clouds in the Magellanic clouds with CII, CI, and CO, , , , , , , , , and . (2017)cite arxiv:1704.00739Comment: 32 pages, 21 figures, Accepted to ApJ.