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1 References  





2 External links  














4U 0614+091






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Coordinates: Sky map06h17m07.3s, +09° 0813
 

From Wikipedia, the free encyclopedia
 


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 06h17m 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[edit]

  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[edit]



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  • Retrieved from "https://en.wikipedia.org/w/index.php?title=4U_0614%2B091&oldid=1184040269"

    Categories: 
    Neutron stars
    X-ray binaries
    Orion (constellation)
    Objects with variable star designations
    Multiple star stubs
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    This page was last edited on 8 November 2023, at 00:07 (UTC).

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