V4641 Sagittarii

V4641 Sagittarii is a variable X-ray binary star system in the constellation Sagittarius. It is the source of one of the fastest superluminal jets in the Milky Way galaxy.

V4641 Sagittarii

A visual band light curve for V4641 Sagittarii, adapted from Goranskij (2001)[1]
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationSagittarius
Right ascension18h 19m 21.63427s[2]
Declination−25° 24′ 25.8493″[2]
Apparent magnitude (V)9.0 - 14.0[3]
Characteristics
Spectral typeB9III[4]
Variable typeHMXB/BHXB/XN+ELL+E[3]
Astrometry
Proper motion (μ) RA: −0.734[2] mas/yr
Dec.: +0.418[2] mas/yr
Parallax (π)0.1510 ± 0.0413 mas[2]
Distance20,200 ± 2,300[4] ly
Orbit[4]
Period (P)2.81730 d
Semi-major axis (a)17.5±1.0 R
Inclination (i)72.3±4.1°
Periastron epoch (T)2,452,423.647
Semi-amplitude (K2)
(secondary)
211.3±1.0 km/s
Details[4]
Black hole
Mass6.4±0.6 M
Stellar companion
Mass2.9±0.4 M
Radius5.3±0.3 R
Surface gravity (log g)3.5±0.1 cgs
Temperature10,250±300 K
Rotational velocity (v sin i)100.9±0.8 km/s
Other designations
V4641 Sgr, GSC 06848-03786, 2MASS J18192163-2524258[5]
Database references
SIMBADdata

In 1999 a violent X-ray outburst revealed it to contain a black hole.[6] At the time, it was considered to be the closest known black hole to Earth, at a distance of approximately 1,600 light-years (490 pc). Later observations showed it to be much farther away, reported in 2001 to be between 7.4 and 12.31 kpc,[7] 6.2 kpc in 2014,[4] and around 6.6 kpc according to its Gaia Data Release 2 parallax.[2]

The star in the binary system is a late B class giant with a mass about three times that of the Sun. It orbits a black hole about twice as massive every 2.8 days. The star is distorted, which causes variations in its brightness as it orbits and rotates. It is also slightly eclipsed by an accretion disc around the black hole. The system usually does not produce a significant amount of x-rays, but undergoes outbursts when the x-ray luminosity increases due to accretion onto the black hole driving superluminal jets.[7]

References