Equinox J2000.0]] (ICRS)
|Right ascension||16h 50m 00.98s|
|Declination||−49° 57′ 43.6″|
XTE J1650-500 is a binary system containing a stellar-mass black hole candidate and 2000–2001 transient binary X-ray source located in the constellation Ara. In 2008, it was claimed that this black hole had a mass of 3.8±0.5 solar masses, which would have been the smallest found for any black hole; smaller than GRO 1655-40, the then known smallest of 6.3 M☉. However, this claim was subsequently retracted; the more likely mass is 5–10 solar masses.
The binary period of the black hole and its companion is 0.32 days.
- "XTE J1650-500". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=XTE+J1650-500.
- Smallest, lightest black hole identified Technology & science - Space - Space.com By Andrea Thompson, updated 4/1/2008 4:32:08 PM ET
- Andrea Thompson (1 April 2008). "Smallest Black Hole Found". Space.com. http://www.space.com/5191-smallest-black-hole.html.
- Determination of Black Hole Masses in Galactic Black Hole Binaries Using Scaling of Spectral and Variability Characteristics Shaposhnikov, Nickolai; Titarchuk, Lev; The Astrophysical Journal, Volume 699, Issue 1, pp. 453-468 (2009) doi:10.1088/0004-637X/699/1/453 Pdf
- Orosz, J.A. et al. (2004) ApJ 616,376-382.
Original source: https://en.wikipedia.org/wiki/ XTE J1650-500. Read more