A method for evaluating models that use galaxy rotation curves to derive the density profiles
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/462/3/2706/8012264/stw1844.pdf
Reference43 articles.
1. NON-NEWTONIAN BEHAVIOR IN WEAK FIELD GENERAL RELATIVITY FOR EXTENDED ROTATING SOURCES
2. Stellar Mass‐to‐Light Ratios and the Tully‐Fisher Relation
3. Binney J. Tremaine S. Galactic Dynamics (Princeton Series in Astrophysics). Princeton Univ. Press; Princeton, NJ; 1988.
4. Too big to fail? The puzzling darkness of massive Milky Way subhaloes
5. The Milky Way’s bright satellites as an apparent failure of ΛCDM
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