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Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic clouds

Tisserand, Patrick; Le Guillou, L; Afonso, C; Albert, J N; Anderson, J; Ansari, R; Aubourg, E; Bareyre, P; Beaulieu, J.-P; Charlot, X; Coutures, C; Ferlet, R; Fouque, P; Glicenstein, J F; Goldman, B; Gould, A; Graff, D.; Gros, M; Haissinski, J; Hamadache, C.; de Kat, J; Lasserre, T; Lesquoy, E; Loup, C; Magneville, C; Marquette, J B; Maurice, E; Maury, A.; Milsztajn, A; Moniez, M; Palanque-Delabrouille, N; Perdereau, O; Rahal, Y R; Rich, J; Spiro, M; Vidal-Madjar, A; Vigroux, L; Zylberajch, S

Description

Aims. The EROS-2 project was designed to test the hypothesis that massive compact halo objects (the so-called "machos") could be a major component of the dark matter halo of the Milky Way galaxy. To this end, EROS-2 monitored over 6.7 years 33 × 106 star

CollectionsANU Research Publications
Date published: 2007
Type: Journal article
URI: http://hdl.handle.net/1885/35144
Source: Astronomy and Astrophysics
DOI: 10.1051/0004-6361:20066017

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