An Upper Limit to the Mass of Black Holes in the Halo of the Galaxy

Keywords

Halo, Globular cluster, Galaxy, Dark matter halo, Dark matter

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Cited by

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• The Dynamics of Galactic WarpsRobert W. Nelson, Scott Tremaine — 1995
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• Towards a direct detection of warm gas in galactic haloes at cosmological distancesMilan M. Ćirković, Joss Bland‐Hawthorn, S. Samurović — 1999
• Effect of Primordial Black Holes on the Cosmic Microwave Background and Cosmological Parameter EstimatesMassimo Ricotti, Jeremiah P. Ostriker, Katherine J. Mack — 2007
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• New cosmological constraints on primordial black holesB. J. Carr, Kazunori Kohri, Yuuiti Sendouda — 2009
• Dynamical constraints on dark compact objects.B. J. Carr — 1998
• Exploring Halo Substructure with Giant Stars. II. Mapping the Extended Structure of the Carina Dwarf Spheroidal GalaxySteven R. Majewski, James C. Ostheimer, Richard J. Patterson — 1999
• THE END OF THE MACHO ERA: LIMITS ON HALO DARK MATTER FROM STELLAR HALO WIDE BINARIESJaiyul Yoo, Julio Chaname, Andrew Gould — 2003
• Canaries in a coal mine: using globular clusters to place limits on massive black holes in the galactic haloPhil Arras, Ira Wasserman — 1998
• A common origin of neutralino stars and supermassive black holesV. I. Dokuchaev, Yu. N. Eroshenko — 2002
• Intermediate-mass black holes in dwarf galaxies: the case of Holmberg IIMichela Mapelli — 2007
• The relationship between X-ray variability and the central black hole massYoujun Lu, Qingjuan Yu — 2001

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