Molecular Clouds in the Extreme Outer Galaxy between l = 34.°75 to 45.°25
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4365/aa63ea/pdf
Reference83 articles.
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1. Erratum: “First Detection of the Molecular Cloud Population in the Extended Ultraviolet Disk of M83” (2022, ApJ, 941, 3);The Astrophysical Journal;2024-07-01
2. A Catalog of 13CO Clumps from the MWISP in l = 10°–20°;Research in Astronomy and Astrophysics;2024-05-01
3. An improved method to measure 12C/13C and 14N/15N abundance ratios: revisiting CN isotopologues in the Galactic outer disc;Monthly Notices of the Royal Astronomical Society;2023-11-27
4. East Asian VLBI Network astrometry toward the extreme outer Galaxy: Kinematic distance with the proper motion of G034.84−00.95;Publications of the Astronomical Society of Japan;2022-12-16
5. First Detection of the Molecular Cloud Population in the Extended Ultraviolet Disk of M83;The Astrophysical Journal;2022-12-01
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