The Origin of [C ii] 157μm Emission in a Five-component Interstellar Medium: The Case of NGC 3184 and NGC 628-Reference-Cited by-同舟云学术

The Origin of [C ii] 157μm Emission in a Five-component Interstellar Medium: The Case of NGC 3184 and NGC 628

Published:2017-06-06 Issue:1 Volume:842 Page:4
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Abdullah A.^ORCID,Brandl B. R.,Groves B.,Wolfire M.,Calzetti D.^ORCID,Croxall K.^ORCID,Looze I. de,Kennicutt R. C.,Sandstrom K. M.^ORCID,Armus L.,Dale D. A.^ORCID,Galametz M.^ORCID,Herrera-Camus R.^ORCID,Hunt L. K.^ORCID,Smith J. D.,Tielens A. G. G. M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/842/i=1/a=4/pdf

Reference138 articles.

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2. MODELING DUST AND STARLIGHT IN GALAXIES OBSERVED BYSPITZERANDHERSCHEL: NGC 628 AND NGC 6946

3. Common-Resolution Convolution Kernels for Space- and Ground-Based Telescopes

4. SHOCK-ENHANCED C+EMISSION AND THE DETECTION OF H2O FROM THE STEPHAN'S QUINTET GROUP-WIDE SHOCK USINGHERSCHEL

5. THE DENSE GAS MASS FRACTION OF MOLECULAR CLOUDS IN THE MILKY WAY

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