41 Aurigae

Binary star system in the constellation Auriga From Wikipedia, the free encyclopedia

41 Aurigae is a binary star[12] system located around 310–316 light years away from the Sun in the northern constellation of Auriga. It is visible to the naked eye as a dim, white-hued star with a combined apparent visual magnitude of 5.83.[12] This system is moving further from the Earth with a heliocentric radial velocity of 31 km/s.[1] It is a probable member of the Hyades Supercluster.[13]

Quick facts Constellation, Right ascension ...
41 Aurigae
Observation data
Epoch J2000      Equinox ICRS
Constellation Auriga[1]
41 Aur A
Right ascension 06h 11m 36.59170s[2]
Declination +48° 42 39.5571[2]
Apparent magnitude (V) 6.15[3]
41 Aur B
Right ascension 06h 11m 36.55276s[4]
Declination +48° 42 47.0365[4]
Apparent magnitude (V) 6.84[3]
Characteristics
41 Aur A
Evolutionary stage Main sequence[2]
Spectral type A2Va+[5]
B−V color index 0.06[3]
41 Aur B
Evolutionary stage main sequence[6]
Spectral type kA5hA5mF0(IV-V)[5]
B−V color index 0.15[3]
Astrometry
41 Aur A
Radial velocity (Rv)31[7] km/s
Proper motion (μ) RA: +14.994[2] mas/yr
Dec.: −55.704[2] mas/yr
Parallax (π)10.6629±0.0539 mas[2]
Distance306 ± 2 ly
(93.8 ± 0.5 pc)
41 Aur B
Radial velocity (Rv)29[7] km/s
Proper motion (μ) RA: +19.171[4] mas/yr
Dec.: −52.460[4] mas/yr
Parallax (π)10.5899±0.0969 mas[4]
Distance308 ± 3 ly
(94.4 ± 0.9 pc)
Details
41 Aur A
Mass2.31[8] M
Radius2.08[8] R
Luminosity27[8] L
Surface gravity (log g)4.17[8] cgs
Temperature9,114[8] K
Rotational velocity (v sin i)138[9] km/s
41 Aur B
Mass1.76[8] M
Radius1.91[8] R
Luminosity11[8] L
Surface gravity (log g)4.13[8] cgs
Temperature7,586[8] K
Rotational velocity (v sin i)133[6] km/s
Other designations
41 Aur, BD+48°1352, HIP 29388, ADS 4773, WDS J06116+4843
41 Aur A: GC 7853, HD 42127, HR 2176, SAO 40925[10]
41 Aur B: GC 7851, HD 42126, HR 2175, SAO 40924[11]
Database references
SIMBAD41 Aur A
41 Aur B
Close

As of 2012, the pair had an angular separation of 7.39 along a position angle of 357.7°.[14] The primary component is an A-type main-sequence star with a stellar classification of A2Va+[5] and a visual magnitude of 6.15.[3] The magnitude 6.84[3] secondary companion is a possible Am star[15] with a stellar classification of kA5hA5mF0(IV-V),[5] showing the calcium K line and hydrogen lines of an A5 star and the metal lines of an F0 star.

References

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