Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Ara |
Right ascension | 16h 50m 00.98s [1] |
Declination | −49° 57′ 43.6″ [1] |
Characteristics | |
Spectral type | K2V [1] |
Astrometry | |
Distance | 3300±700 [2] pc |
Details | |
Black hole | |
Mass | 9.7±1.6 [2] M☉ |
Other designations | |
INTREF 720 | |
Database references | |
SIMBAD | data |
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, [3] which would have been the smallest found for any black hole; smaller than GRO 1655−40, the then known smallest of 6.3 M☉. [4] However, this claim was subsequently retracted; [2] the more likely mass is 5–10 solar masses.
The binary period of the black hole and its companion is 0.32 days. [5]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Ara |
Right ascension | 16h 50m 00.98s [1] |
Declination | −49° 57′ 43.6″ [1] |
Characteristics | |
Spectral type | K2V [1] |
Astrometry | |
Distance | 3300±700 [2] pc |
Details | |
Black hole | |
Mass | 9.7±1.6 [2] M☉ |
Other designations | |
INTREF 720 | |
Database references | |
SIMBAD | data |
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, [3] which would have been the smallest found for any black hole; smaller than GRO 1655−40, the then known smallest of 6.3 M☉. [4] However, this claim was subsequently retracted; [2] the more likely mass is 5–10 solar masses.
The binary period of the black hole and its companion is 0.32 days. [5]