Testing Modified Gravity with Globular Cluster Velocity Dispersions

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Testing Modified Gravity with Globular Cluster Velocity Dispersions

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ar X iv : 0 70 8 . 19 35 v 3 [ as tr o - ph ] 2 7 A ug 2 00 7 Testing modified gravity with globular cluster velocity dispersions

Globular clusters (GCs) in the Milky Way have characteristic velocity dispersions that are consistent with the predictions of Newtonian gravity, and may be at odds with Modified Newtonian Dynamics (MOND) and possibly the cold dark matter model. We discuss a modified gravity (MOG) theory that can successfully model the velocity dispersions of GCs in the Galactic neighborhood. MOG produces veloci...

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ar X iv : 0 70 8 . 19 35 v 2 [ as tr o - ph ] 1 6 A ug 2 00 7 Testing modified gravity with globular cluster velocity dispersions

Globular clusters in the Milky Way have characteristic velocity dispersions that are consistent with the predictions of Newtonian gravity, and may be at odds with Modified Newtonian Dynamics (MOND) and possibly the cold dark matter model. We discuss a modified gravity (MOG) theory that can successfully model the velocity dispersions of GCs in the Galactic neighborhood. MOG produces velocity dis...

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ar X iv : 0 70 8 . 19 35 v 1 [ as tr o - ph ] 1 4 A ug 2 00 7 Testing modified gravity with globular cluster velocity dispersions

Globular clusters in the Milky Way have characteristic velocity dispersions that are consistent with the predictions of Newtonian gravity, and may be at odds with Modified Newtonian Dynamics (MOND) and possibly the cold dark matter model. We discuss a modified gravity (MOG) theory that can successfully model the velocity dispersions of GCs in the Galactic neighborhood. MOG produces velocity dis...

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ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 2008

ISSN: 0004-637X,1538-4357

DOI: 10.1086/587926