The formation of spiral galaxies: adiabatic compression with Young's algorithm and the relation of dark matter haloes to their primordial antecedents
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/439/2/1897/18471918/stu070.pdf
Reference55 articles.
1. Simulations of Galaxy Formation in a Λ Cold Dark Matter Universe. I. Dynamical and Photometric Properties of a Simulated Disk Galaxy
2. Halo Response to Galaxy Formation
3. Stellar Mass‐to‐Light Ratios and the Tully‐Fisher Relation
4. Contraction of dark matter galactic halos due to baryonic infall
5. A DIRECT DYNAMICAL MEASUREMENT OF THE MILKY WAY'S DISK SURFACE DENSITY PROFILE, DISK SCALE LENGTH, AND DARK MATTER PROFILE AT 4 kpc ≲R≲ 9 kpc
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