SMA OBSERVATIONS OF THE EXTENDED12CO(J= 6–5) EMISSION IN THE STARBURST GALAXY NGC 253
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/821/i=2/a=112/pdf
Reference73 articles.
1. Aλ= 1.3 mm and 2 mm molecular line survey towards M 82
2. The submillimeter C and CO lines in Henize 2-10 and NGC 253
3. ALMA observations of 99 GHz free–free and H40α line emission from star formation in the centre of NGC 253
4. Submillimeter Array 440 μm/690 GHz Line and Continuum Observations of Orion KL
5. Suppression of star formation in the galaxy NGC 253 by a starburst-driven molecular wind
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1. Atomic Carbon in the Central Molecular Zone of the Milky Way: Possible Cosmic-Ray Induced Chemistry or Time-dependent Chemistry Associated with SNR Sagittarius A East;The Astrophysical Journal;2021-07-01
2. ALMA view of the 12C/13C isotopic ratio in starburst galaxies;Astronomy & Astrophysics;2019-08-22
3. Spatially resolved carbon and oxygen isotopic ratios in NGC 253 using optically thin tracers;Astronomy & Astrophysics;2019-04
4. Diverse Nuclear Star-forming Activities in the Heart of NGC 253 Resolved with 10-pc-scale ALMA Images;The Astrophysical Journal;2017-11-06
5. Molecular gas properties of a lensed star-forming galaxy at z ~ 3.6: a case study;Astronomy & Astrophysics;2017-09
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