Characterizing the Transition from Diffuse Atomic to Dense Molecular Clouds in the Magellanic Clouds with [C ii], [C i], and CO-Reference-Cited by-同舟云学术

Characterizing the Transition from Diffuse Atomic to Dense Molecular Clouds in the Magellanic Clouds with [C ii], [C i], and CO

Published:2017-04-21 Issue:2 Volume:839 Page:107
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Pineda Jorge L.^ORCID,Langer William D.,Goldsmith Paul F.^ORCID,Horiuchi Shinji,Kuiper Thomas B. H.^ORCID,Muller Erik,Hughes Annie,Ott Jürgen^ORCID,Requena-Torres Miguel A.,Velusamy Thangasamy,Wong Tony^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/839/i=2/a=107/pdf

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4. ANALYTIC H i-to-H2 PHOTODISSOCIATION TRANSITION PROFILES

5. The Role of Pressure in GMC Formation II: The H2‐Pressure Relation

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