XTE J1650-500 ~ Low Mass X-ray Binary

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 MSun. 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.

Source : Wikipedia 

Coordinates : SIMBAD 

Article About XTE J1650-500 : Stargate 







XTE J1650-500 Low Mass X-ray Binary.kmz (1.18 KB)