Atomic and molecular gas in the starburst galaxy NGC 4945
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20010505/pdf
Reference67 articles.
1. A New High‐Resolution CO Map of the Inner 2.́5 of M51. I. Streaming Motions and Spiral Structure
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3. Powerful extragalactic masers
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5. Begeman, K. 1987, Ph.D. Thesis, Rijksuniversiteit te Groningen, The Netherlands
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1. Hot Gas Outflow Properties of the Starburst Galaxy NGC 4945;The Astrophysical Journal;2024-06-01
2. The extended H i halo of NGC 4945 as seen by MeerKAT;Monthly Notices of the Royal Astronomical Society;2022-04-07
3. The diffuse γ-ray background is dominated by star-forming galaxies;Nature;2021-09-15
4. The multi-phase ISM in the nearby composite AGN-SB galaxy NGC 4945: large-scale (parsecs) mechanical heating;Astronomy & Astrophysics;2020-10
5. Discovery of a transient X-ray source Suzaku J1305−4930 in NGC 4945;Publications of the Astronomical Society of Japan;2020-05-12
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