Arp 220: New Observational Insights into the Structure and Kinematics of the Nuclear Molecular Disks and Surrounding Gas
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab8f32/pdf
Reference51 articles.
1. Probing highly obscured, self-absorbed galaxy nuclei with vibrationally excited HCN
2. The hidden heart of the luminous infrared galaxy IC 860
3. Overluminous HNC line emission in Arp 220, NGC 4418 and Mrk 231. Global IR pumping or XDRs?
4. Fast, Collimated Outflow in the Western Nucleus of Arp 220
5. HIGH-RESOLUTION RADIO CONTINUUM MEASUREMENTS OF THE NUCLEAR DISKS OF Arp 220
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1. The OH Megamaser emission in Arp 220: the rest of the story;Monthly Notices of the Royal Astronomical Society;2023-06-16
2. Arp 220: A Post-starburst Galaxy with Little Current Star Formation outside of Its Nuclear Disks;The Astrophysical Journal;2023-02-01
3. The Extremely Buried Nucleus of IRAS 17208–0014 Observed at Submillimeter and Near-infrared Wavelengths;The Astrophysical Journal;2022-04-01
4. Spatially-resolved relation between [C i] 3P1–3P0 and 12CO (1–0) in Arp 220;Publications of the Astronomical Society of Japan;2022-03-16
5. Deeply Buried Nuclei in the Infrared-luminous Galaxies NGC 4418 and Arp 220. II. Line Forests at λ = 1.4–0.4 mm and Circumnuclear Gas Observed with ALMA;The Astrophysical Journal;2021-12-01
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