XTE J1650−500: Difference between revisions
Content deleted Content added
iw |
SilvonenBot (talk | contribs) m robot Adding: pl:XTE J1650-500 |
||
| Line 12: | Line 12: | ||
{{astronomy-stub}} |
{{astronomy-stub}} |
||
[[de:XTE J1650-500]] |
[[de:XTE J1650-500]] |
||
[[es:J1650–500]] |
[[es:J1650–500]] |
||
[[pl:XTE J1650-500]] |
|||
[[fi:J1650]] |
[[fi:J1650]] |
||
Revision as of 14:25, 21 July 2008
XTE J1650-500 is a stellar-mass black hole candidate and 2000-2001 transient binary X-ray source located in the constellation Ara. Its mass of 3.8±0.5 solar masses[1] is the smallest yet found for any black hole, and near the theoretical upper mass limit (~2.7 solar masses) for a neutron star. The binary period is 0.32 days[1].
See also
References
- ^ Orosz, J.A. et al. (2004) ApJ 616,376-382.
 | This astronomy-related article is a stub. You can help Wikipedia by expanding it. |