Theory of pixel lensing toward M31. II. The velocity anisotropy and flattening of the MACHO distribution

Astrophysical Journal

Volumn 598, Issue 2 I, 2003, Pages 993-999

  Kerins, E ^a   An, J ^b   Evans, N W ^b   Baillon, P ^c   Carr, B J ^d   Giraud Heraud Y ^e   Gould, A ^f   Hewett, P ^b   Kaplan, J ^e   Paulin Henriksson, S ^e   Smartt, S J ^b   Tsapras, Y ^d   Valls Gabaud, D ^g  

^a LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^c CERN   (Switzerland)

^d QUEEN MARY UNIVERSITY OF LONDON   (United Kingdom)

^e Grp de Biol de la Cellule N   (France)

^f OHIO STATE UNIVERSITY   (United States)

^g IRAP   (France)

Author keywords

Dark matter; Galaxies: individual (M31); Gravitational lensing

Indexed keywords

EID: 18544396161     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/379060     Document Type: Article

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