Enhanced H iprofile asymmetries in close galaxy pairs

Author:

Bok J12,Blyth S-L2,Gilbank D G13ORCID,Elson E C45ORCID

Affiliation:

1. South African Astronomical Observatory, Observatory, Cape Town 7935, South Africa

2. Department of Astronomy, University of Cape Town, Private Bag X3, Rondebosch 7700, South Africa

3. Centre for Space Research, North-West University, Potchefstroom, 2520 Cape Town, South Africa

4. Department of Physics and Astronomy, University of the Western Cape, Robert Sobukwe Rd, Bellville, Cape Town 7535, South Africa

5. South African Radio Astronomy Observatory (SARAO), 2 Fir Street, Black River Park, Observatory 7925, South Africa

Funder

National Science Foundation

University of Cape Town

University of Basel

University of Cambridge

Case Western Reserve University

University of Chicago

Drexel University

Johns Hopkins University

New Mexico State University

Ohio State University

University of Pittsburgh

University of Portsmouth

Princeton University

United States Naval Observatory

University of Washington

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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1. Shape Asymmetries and the Relation between Lopsidedness and Radial Alignment in Simulated Galaxies;The Astrophysical Journal;2024-01-01

2. Measuring galaxy asymmetries in 3D;Monthly Notices of the Royal Astronomical Society;2023-06-08

3. A Generalist, Automated ALFALFA Baryonic Tully–Fisher Relation;The Astrophysical Journal;2023-06-01

4. Inferring dark matter halo properties for H i-selected galaxies;Monthly Notices of the Royal Astronomical Society;2023-05-09

5. SAMI-H i: the connection between global asymmetry in the ionized and neutral atomic hydrogen gas in galaxies;Monthly Notices of the Royal Astronomical Society;2022-12-16

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