4U 0614+091

Binary star in the constellation Orion
4U 0614+091

A broadband optical light curve for V1055 Orionis, adapted from Zhang et al. (2012)[1]
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
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)6 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. arXiv:1110.1267. doi:10.1111/j.1365-2966.2011.19935.x. S2CID 119279347.

External links

  • Astrophysicists Discover Compact Jets From Neutron Star – Space Daily
  • Surprising Activity from a Dead Star – Space.com
  • V1055 Ori


  • v
  • t
  • e
Constellation of Orion
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star
clusters
NGC
Other
Nebulae
NGC
Other
Galaxies
NGC
Other
Astronomical events
  • GRB 991216
Category


Stub icon

This binary or multiple star system-related article is a stub. You can help Wikipedia by expanding it.

  • v
  • t
  • e