Astronomy:4U 0614+091

From HandWiki
Short description: Binary star in the constellation Orion
4U 0614+091
V1055OriLightCurve.png
A broadband optical light curve for V1055 Orionis, adapted from Zhang et al. (2012)[1]
Observation data
Epoch J2000.0   Equinox (celestial coordinates)
Constellation Orion
Right ascension  06h 17m 07.3s
Declination +09° 08′ 13″
Apparent magnitude (V) 18.8
Characteristics
U−B color index 18.5
B−V color index 18.8
Astrometry
Proper motion (μ) RA: 94.28084 mas/yr
Dec.: +9.13667 mas/yr
Parallax (π)mas
Distance10,000 ly
(3,000 pc)
Absolute magnitude (MV)19.8
Other designations
1RXS J061707.4+090812, V1055 Ori
Database references
SIMBADdata

4U 0614+091 is a low-mass X-ray binary star system which features a neutron star and a low-mass companion star. The binary system lies 10,000 light-years away in Orion. It produces jets like a microquasar, the first time an object other than a black hole has been shown to produce jets.

References

  1. Zhang, Y.; Hynes, R. I.; Robinson, E. L. (February 2012). "Millihertz quasi-periodic optical oscillations in 4U 0614+091". Monthly Notices of the Royal Astronomical Society 419 (4): 2943–2948. doi:10.1111/j.1365-2966.2011.19935.x. 

External links

Coordinates: Sky map 06h 17m 07.3s, +09° 08′ 13″