The baryonic Tully–Fisher relation for different velocity definitions and implications for galaxy angular momentum-Reference-Cited by-同舟云学术

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The baryonic Tully–Fisher relation for different velocity definitions and implications for galaxy angular momentum

Published:2019-01-18 Issue:3 Volume:484 Page:3267-3278
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Lelli Federico¹^ORCID,McGaugh Stacy S²,Schombert James M³,Desmond Harry⁴^ORCID,Katz Harley⁴

Affiliation:

1. European Southern Observatory, Karl-Schwarschild-Strasse 2, 85748 Garching bei München, Germany

2. Department of Astronomy, Case Western Reserve University, Cleveland, OH 44106, USA

3. Department of Physics, University of Oregon, Eugene, OR 97403, USA

4. Astrophysics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/484/3/3267/27711809/stz205.pdf

Reference71 articles.

1. A SLIPPERY SLOPE: SYSTEMATIC UNCERTAINTIES IN THE LINE WIDTH BARYONIC TULLY–FISHER RELATION

2. The different baryonic Tully–Fisher relations at low masses

3. The ATLAS3D project – XV. Benchmark for early-type galaxies scaling relations from 260 dynamical models: mass-to-light ratio, dark matter, Fundamental Plane and Mass Plane

4. VLA IMAGING OF VIRGO SPIRALS IN ATOMIC GAS (VIVA). I. THE ATLAS AND THE H I PROPERTIES

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