4U 0614+091

{{Short description|Binary star in the constellation Orion}}

{{no footnotes|date=March 2017}}

{{Starbox begin |

name=4U 0614+091}}

{{Starbox image

| image = 250px

| caption = A broadband optical light curve for V1055 Orionis, adapted from Zhang et al. (2012)

}}

{{Starbox observe |

epoch=J2000.0 (ICRS) |

ra={{RA|06|17|07.3}} |

dec={{DEC|+09|08|13}} |

appmag_v=18.8 |

constell=Orion }}

{{Starbox character |

class= |

b-v= 18.8 |

u-b= 18.5|

variable=

}}

{{Starbox astrometry |

radial_v= |

prop_mo_ra= 94.28084 |

prop_mo_dec= +9.13667|

parallax= 6 |

dist_ly = 10,000|

dist_pc = 3,000 |

p_error= |

absmag_v= 19.8}}

{{Starbox catalog |

names= 1RXS J061707.4+090812, V1055 Ori }}

{{Starbox reference

|Simbad=V1055+Ori

}}

{{Starbox end}}

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.