Mahasim
Double star Mahasim (θ Aurigae) |
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AladinLite | |||||||||||||||||||||
Observation dates equinox : J2000.0 , epoch : J2000.0 |
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Constellation | Carter | ||||||||||||||||||||
Right ascension | 05 h 59 m 43.27 s | ||||||||||||||||||||
declination | + 37 ° 12 ′ 45.3 ″ | ||||||||||||||||||||
Apparent brightness | 2.62 to 2.70 mag | ||||||||||||||||||||
Typing | |||||||||||||||||||||
B − V color index | (−0.08) | ||||||||||||||||||||
U − B color index | (−0.18) | ||||||||||||||||||||
R − I index | (−0.06) | ||||||||||||||||||||
Spectral class | A0pSi / F2-5 V | ||||||||||||||||||||
Variable star type | ACV | ||||||||||||||||||||
Astrometry | |||||||||||||||||||||
Radial velocity | (29.3 ± 1.7) km / s | ||||||||||||||||||||
parallax | (19.70 ± 0.16) mas | ||||||||||||||||||||
distance | (165 ± 2) ly (51) pc |
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Proper movement | |||||||||||||||||||||
Rec. Share: | (43.63 ± 0.21) mas / a | ||||||||||||||||||||
Dec. portion: | (−73.79 ± 0.08) mas / a | ||||||||||||||||||||
Physical Properties | |||||||||||||||||||||
radius | (5.1 ± 0.4) R ☉ | ||||||||||||||||||||
Effective temperature | (10400 ± 300) K. | ||||||||||||||||||||
Rotation time | 3.62 d | ||||||||||||||||||||
Other names and catalog entries |
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Mahasim is an Ap star in the constellation Fuhrmann, about 170 light years away, with an apparent magnitude of around 2.7 mag. A companion star of the spectral class F2-5 V with an apparent magnitude of 7.2 mag is located at a distance of just under 4 arc seconds .
The star also bears the historical proper name Bogardus and - in traditional Chinese astronomy - 五 車 四.
swell
- Adelman, SJ; Hensberge, H .; van Rensbergen, W .: General study of the apparently average magnetic Ap star theta Aurigae. I. Data and method ; in: Astronomy and Astrophysics Supplement Series ( ISSN 0365-0138 ), Vol. 57, pp. 121ff. (July 1984), bibcode : 1984A & AS ... 57..121A
Web links
Individual evidence
- ↑ a b c d e f tet Aur. In: SIMBAD . Center de Données astronomiques de Strasbourg , accessed September 8, 2018 .
- ↑ a b C. Schröder, JHMM Schmitt: X-ray emission from A-type stars . In: Astronomy and Astrophysics . 475, No. 2, November 2007, pp. 677-684. bibcode : 2007A & A ... 475..677S . doi : 10.1051 / 0004-6361: 20077429 .
- ↑ a b tet Aur. In: VSX. AAVSO, accessed September 8, 2018 .
- ↑ a b D. Shulyak, G. Valyavin, O. Kochukhov, B.-C. Lee, G. Galazutdinov, K.-M. Kim, I. Han, T. Burlakova, V. Tsymbal: The Lorentz force in atmospheres of CP stars: θ Aurigae . In: Astronomy & Astrophysics . 464, No. 3, March 2007, pp. 1089-1099. arxiv : astro-ph / 0612301 . bibcode : 2007A & A ... 464.1089S . doi : 10.1051 / 0004-6361: 20064998 .
- ↑ JB Rice, DE Holmgren, DA Bohlender: The distribution of oxygen on the surface of the Ap star θ Aur. An abundance Doppler image to compare with ɛ UMa . In: Astronomy and Astrophysics . 424, September 2004, pp. 237-244. bibcode : 2004A & A ... 424..237R . doi : 10.1051 / 0004-6361: 20035639 .
- ↑ List of names verified by the IAU