Disentangling the ISM phases of the dwarf galaxy NGC 4214 using [C ii] SOFIA/GREAT observations-Reference-Cited by-同舟云学术

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Disentangling the ISM phases of the dwarf galaxy NGC 4214 using [C ii] SOFIA/GREAT observations

Published:2017-02-20 Issue: Volume:599 Page:A9
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Fahrion K.,Cormier D.,Bigiel F.,Hony S.,Abel N. P.,Cigan P.,Csengeri T.,Graf U. U.,Lebouteiller V.,Madden S. C.,Wu R.,Young L.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201629341/pdf

Reference54 articles.

1. The CO-to-H2 Conversion Factor

2. Spectrally resolved C II emission in M 33 (HerM33es)

3. HERSCHEL SPECTROSCOPIC OBSERVATIONS OF LITTLE THINGS DWARF GALAXIES

4. The effects of star formation on the low-metallicity ISM: NGC 4214 mapped withHerschel/PACS spectroscopy

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1. The Interstellar Medium in Dwarf Irregular Galaxies;Annual Review of Astronomy and Astrophysics;2024-09-13

2. COLDSIM predictions of [C II] emission in primordial galaxies;Astronomy & Astrophysics;2024-09

3. Spectral study of X-ray sources in some galaxies recently observed by Chandra;Indian Journal of Physics;2024-03-05

4. [C ii] 158 μm emission as an indicator of galaxy star formation rate;Monthly Notices of the Royal Astronomical Society;2023-12-11

5. [C ii] Spectral Mapping of the Galactic Wind and Starbursting Disk of M82 with SOFIA;The Astrophysical Journal;2023-11-16

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