What makes the family of barred disc galaxies so rich: damping stellar bars in spinning haloes-Reference-Cited by-同舟云学术

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What makes the family of barred disc galaxies so rich: damping stellar bars in spinning haloes

Published:2018-02-02 Issue:1 Volume:476 Page:1331-1344
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Collier Angela¹,Shlosman Isaac¹²,Heller Clayton³

Affiliation:

1. Department of Physics and Astronomy, University of Kentucky, Lexington, KY 40506-0055, USA

2. Theoretical Astrophysics, Graduate School of Science, Osaka University, Osaka 560-0043, Japan

3. Department of Physics, Georgia Southern University, Statesboro, GA 30460, USA

Funder

JSPS

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/476/1/1331/24275481/sty270.pdf

Reference63 articles.

1. The shape of dark matter haloes: dependence on mass, redshift, radius and formation

2. The existence and shapes of dust lanes in galactic bars

3. What determines the strength and the slowdown rate of bars?

4. On the nature of bulges in general and of box/peanut bulges in particular: input fromN-body simulations

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1. Metal-poor Stars in the MW Disk: Resonant Cooling of Vertical Oscillations of Halo Stars in Barred Galaxies;The Astrophysical Journal Letters;2024-08-01

2. Effects of Halo Spin on the Formation and Evolution of Bars in Disk Galaxies;The Astrophysical Journal;2024-08-01

3. Importance of Initial Condition on Bar Secular Evolution: Role of Halo Angular Momentum Distribution Discontinuity;The Astrophysical Journal;2024-07-01

4. The Rotation of Classical Bulges in Barred Galaxies in the Presence of Gas;Universe;2024-05-16

5. Positive Lynden-Bell derivative as a ticket to the bar trap?;Monthly Notices of the Royal Astronomical Society;2024-03-08

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