arXiv Analytics

Sign in

arXiv:1312.6475 [astro-ph.GA]AbstractReferencesReviewsResources

Polar rings and the 3D-shape of dark matter

Francoise Combes

Published 2013-12-23Version 1

Polar ring galaxies (PRG) are unique to give insight on the 3D-shape of dark matter haloes. Some caveats have prevented to draw clear conclusions in previous works. Also the formation mechanisms need to be well known. All available information on the topic is reviewed, and criteria are defined for an ideal PRG system, in the hope of removing the ambiguities and make progress in the domain.

Comments: 8 pages, 4 figures, Proceedings of "Multi-spin galaxies", Napoli October 2013, E. Iodice, Ed
Categories: astro-ph.GA, astro-ph.CO
Related articles: Most relevant | Search more
arXiv:2206.07069 [astro-ph.GA] (Published 2022-06-14)
The Response of Dark Matter Haloes to Gas Ejection: CuspCore II
arXiv:1811.12839 [astro-ph.GA] (Published 2018-11-30)
Major Mergers between Dark Matter Haloes -- I: Predictions for Size, Shape and Spin
arXiv:2501.13015 [astro-ph.GA] (Published 2025-01-22)
Constraining the shape of dark matter haloes using only starlight. I. A new technique and its application to the galaxy Nube