Spiral structure in barred galaxies. Observational constraints to spiral arm formation mechanisms-Reference-Cited by-同舟云学术

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Spiral structure in barred galaxies. Observational constraints to spiral arm formation mechanisms

Published:2018-11-03 Issue:4 Volume:482 Page:5362-5378
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Font Joan¹²,Beckman John E¹²³,James Phil A⁴,Patsis Panos A⁵

Affiliation:

1. Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain

2. Departamento de Astrofísica, Universidad de La Laguna, La Laguna, Tenerife, Spain

3. Consejo Superior de Investigaciones Científicas, Spain

4. Astrophysics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park, 146 Brownlow Hill, Liverpool L3 5RF, UK

5. Research Center for Astronomy, Academy of Athens, Soranou Efessiou 4, GR-115 27 Athens, Greece

Funder

Instituto de Astrofsica de Canarias

Alfred P. Sloan Foundation

National Science Foundation

U.S. Department of Energy

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/482/4/5362/26917339/sty2983.pdf

Reference112 articles.

1. Morphology of bar orbits

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

3. Manifold-driven spirals inN-body barred galaxy simulations

4. Bars and secular evolution in disk galaxies: Theoretical input

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