Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Auriga |
Right ascension | 05h 27m 52.40539s[2] |
Declination | +34° 46′ 58.3435″[2] |
Apparent magnitude (V) | 8.19 to 8.83[3] |
Characteristics | |
Spectral type | B0p + B1Vp[3] + ? |
U−B color index | -0.66 |
B−V color index | 0.18 |
Variable type | Eclipsing binary[4] |
Astrometry | |
Radial velocity (Rv) | 9 ± 5 km/s |
Proper motion (μ) | RA: −4.479[2] mas/yr Dec.: -9.049[2] mas/yr |
Parallax (π) | 0.4786 ± 0.5765 mas[2] |
Other designations | |
Database references | |
SIMBAD | data |
IU Aurigae is a triple star[6] system in the constellation Auriga, consisting of an eclipsing binary pair orbiting a third component with a period of 335 years.[7] This system is too faint to be viewed with the naked eye, having a peak apparent visual magnitude of 8.19.[3] The eclipsing pair form a Beta Lyrae-type semidetached binary of two Bp stars[3] with a period of 1.81147435 days.[4] During the primary eclipse, the visual magnitude of the system drops to 8.89, while for the secondary it decreases to 8.74.[3][8] The third component is a massive object with 17–18 M☉, and may actually be a binary – which would make this a quadruple star system.[7]
Özdemir
was invoked but never defined (see the help page).GaiaDR2
was invoked but never defined (see the help page).Avvakumova2013
was invoked but never defined (see the help page).Samus2017
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).Mayer1987
was invoked but never defined (see the help page).Drechsel1994
was invoked but never defined (see the help page).AAVSOIU
was invoked but never defined (see the help page).