A correlation between the H i 21-cm absorption strength and impact parameter in external galaxies
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/459/4/4136/8192268/stw943.pdf
Reference52 articles.
1. Discovery of H i gas in a young radio galaxy at z = 0.44 using the Australian Square Kilometre Array Pathfinder
2. USING 21 cm ABSORPTION IN SMALL IMPACT PARAMETER GALAXY-QUASAR PAIRS TO PROBE LOW-REDSHIFT DAMPED AND SUB-DAMPED Lyα SYSTEMS
3. A GREEN BANK TELESCOPE SURVEY FOR H I 21 cm ABSORPTION IN THE DISKS AND HALOS OF LOW-REDSHIFT GALAXIES
4. Borthakur S. Momjian E. Heckman T. M. York D. G. Bowen D. V. Yun M. S. Tripp T. M. ApJ 2014:98.
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2. The First Large Absorption Survey in H i (FLASH): I. Science goals and survey design;Publications of the Astronomical Society of Australia;2022
3. Intervening or associated? Machine learning classification of redshifted H i 21-cm absorption;Monthly Notices of the Royal Astronomical Society;2021-07-02
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5. Low-mass Group Environments Have No Substantial Impact on the Circumgalactic Medium Metallicity;The Astronomical Journal;2020-04-16
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