Star formation and bar instability in cosmological halos

2008/01/30 by A. Curir, Anna Curir, Paola Mazzei +2 · 1 citation
Physics and Astronomy · #Astrophysics and Star Formation Studies #Galaxies: Formation, Evolution, Phenomena #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20078285

10 pages, 21 figures, A&A accepted

arxiv created 2008/01/30 · openalex publication_date 2008/02/18 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/31

Abstract

Context. This is the third in a series of papers presenting the first attempt to analyse the growth of the bar instability in a consistent cosmological scenario. In the previous two articles, we explored the role of the cosmology on stellar disks and the impact of the gaseous component on a disk embedded in a cosmological dark matter halo.

Citations

• Numerical recipes: the art of scientific computing

Cited by

• Evolution and instabilities of disks harboring super massive black holes

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