Search for nearby counterparts to the moving objects in the Hubble Deep Field

被引:26
|
作者
Flynn, C [1 ]
Sommer-Larsen, J
Fuchs, B
Graff, DS
Salim, S
机构
[1] Tuorla Observ, FIN-21500 Piikkio, Finland
[2] Theoret Astrophys Ctr, Copenhagen, Denmark
[3] Astron Rech Inst, D-6900 Heidelberg, Germany
[4] Ohio State Univ, Dept Phys, Columbus, OH 43210 USA
[5] Ohio State Univ, Dept Astron, Columbus, OH 43210 USA
关键词
Galaxy : structure; dark matter;
D O I
10.1046/j.1365-8711.2001.04082.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Ibata et al. have recently discovered very faint, moving objects in the Hubble Deep Field (HDF). The number, apparent magnitudes and proper motions of these objects are consistent with old white dwarfs making up part of the Galactic dark halo. We review a number of ground-based proper motion surveys in which nearby dark-halo white dwarfs might be present, if they have the colours and absolute magnitudes proposed. No such objects have been found, whereas we argue here that several times more would be expected than in the HDF. We conclude that it is unlikely that hydrogen-atmosphere white dwarfs make up a significant fraction of the Galactic dark matter. No limits can be placed as yet on helium-atmosphere dwarfs from optical searches.
引用
收藏
页码:553 / 560
页数:8
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