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      MACHO Project Limits on Black Hole Dark Matter in the 1–30 [ITAL]M[/ITAL][TINF]⊙[/TINF] Range

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          The MACHO Project Large Magellanic Cloud Microlensing Results from the First Two Years and the Nature of the Galactic Dark Halo

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            Primordial black hole formation during the QCD epoch

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              Galactic microlensing as a method of detecting massive compact halo objects

              Kim Griest (1991)
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                Author and article information

                Journal
                The Astrophysical Journal
                University of Chicago Press
                0004637X
                April 1 2001
                : 550
                : 2
                : L169-L172
                Article
                10.1086/319636
                9d08fbf0-324f-40ef-8cdb-88ed3195bf25
                © 2001
                History

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