Velocity resolved [C ii], [C i], and CO observations of the N159 star-forming region in the Large Magellanic Cloud: a complex velocity structure and variation of the column densities-Reference-Cited by-同舟云学术

Velocity resolved [C ii], [C i], and CO observations of the N159 star-forming region in the Large Magellanic Cloud: a complex velocity structure and variation of the column densities

Published:2015-07-30 Issue: Volume:580 Page:A54
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Okada Yoko,Requena-Torres Miguel Angel,Güsten Rolf,Stutzki Jürgen,Wiesemeyer Helmut,Pütz Patrick,Ricken Oliver

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201525630/pdf

Reference72 articles.

1. The H ii Region/PDR Connection: Self‐consistent Calculations of Physical Conditions in Star‐forming Regions

2. The photoelectric heating mechanism for very small graphitic grains and polycyclic aromatic hydrocarbons

3. A Semianalytical Model for the Observational Properties of the Dominant Carbon Species at Different Metallicities

4. Carbon in the N159/N160 Complex of the Large Magellanic Cloud

5. Ionized carbon in the Large Magellanic Cloud

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