CO (J = 7→6) Observations of NGC 253: Cosmic‐Ray–heated Warm Molecular Gas-Reference-Cited by-同舟云学术

CO (J = 7→6) Observations of NGC 253: Cosmic‐Ray–heated Warm Molecular Gas

Published:2003-04 Issue:2 Volume:586 Page:891-901
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Bradford C. M.,Nikola T.,Stacey G. J.,Bolatto A. D.,Jackson J. M.,Savage M. L.,Davidson J. A.,Higdon S. J.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/586/i=2/a=891/pdf

Reference58 articles.

1. A large family of compact radio sources in the starburst nucleus of NGC 253

2. SPIFI: a direct-detection imaging spectrometer for submillimeter wavelengths

3. The molecular gas bar in NGC 253

4. Carlstrom, J. E., Jackson, J., Ho, P. T. P. & Turner, J. L. 1990, in The Interstellar Medium in External Galaxies: Summaries of Contributed Papers, ed. D. J. Hollenbach & H. A. Thronson (Washington: NASA), 337

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