A solution for galactic disks with Yukawian gravitational potential
Author:
Publisher
Springer Science and Business Media LLC
Subject
Physics and Astronomy (miscellaneous)
Link
http://link.springer.com/content/pdf/10.1007/s10714-007-0420-8.pdf
Reference17 articles.
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2. Piazza F. and Marinoni C. (2003). Model for gravitational interaction between dark matter and baryons. Phys. Rev. Lett. 91: 141301
3. Rodríguez-Meza M.A. (2005). Potential density pairs for axisymmetric galaxies: the influence of scalar fields. Gen. Relativ. Gravit. 37: 823
4. Signore R.L. (2005). Non-Newtonian potential involving Hubble’s length. Mon. Not. R. Astron. Soc. 364: 1219
5. Freeman K.C. (1970). On the disks of spiral and S0 galaxies. Astrophys. J. 160: 811
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