astro.wikisort.org - StarOU Geminorum (OU Gem) is a visual binary or possible triple star located in the constellation of Gemini.
Multiple star system in the constellation Gemini
OU Geminorum
 A visual band light curve for OU Geminorum, adapted from Bopp et al. (1981) [1] |
Observation data Epoch J2000 Equinox J2000 |
Constellation |
Gemini |
Right ascension |
06h 26m 10.2464s[2] |
Declination |
+18° 45′ 24.896″[2] |
Apparent magnitude (V) |
6.768[3] |
Characteristics |
Spectral type |
K3Vk[3] |
U−B color index |
0.662[3] |
B−V color index |
0.972[3] |
Variable type |
BY Dra[4] |
Astrometry |
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Radial velocity (Rv) | −8.98±0.10[5] km/s |
Proper motion (μ) | RA: −124.020±0.097[2] mas/yr Dec.: −159.335±0.054[2] mas/yr |
Parallax (π) | 68.46 ± 0.34 mas[2] |
Distance | 47.6 ± 0.2 ly (14.61 ± 0.07 pc) |
Absolute magnitude (MV) | 5.93±0.05[3] |
|
Orbit[5] |
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Primary | OU Gem Aa |
Companion | OU Gem Ab |
Period (P) | 6.991878±0.000004 d |
Eccentricity (e) | 0.151±0.0024 |
Periastron epoch (T) | 54900.0719±0.0203 JD |
Argument of periastron (ω) (secondary) | 77.63±1.09° |
Semi-amplitude (K1) (primary) | 57.09±0.15 km/s |
Semi-amplitude (K2) (secondary) | 66.22±0.28 km/s |
Details[6] |
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OU Gem Aa |
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Mass | 0.85 M☉ |
Radius | 0.81 R☉ |
Surface gravity (log g) | 4.55 cgs |
Temperature | 4960 K |
OU Gem Ab |
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Mass | 0.71 M☉ |
Radius | 0.65 R☉ |
Surface gravity (log g) | 4.65 cgs |
Temperature | 4390 K |
Other designations |
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OU Gem, BD+18 1214, GJ 233, HD 45088, HIP 30630, SAO 95677. [7] |
Database references |
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SIMBAD | data |
The system has an absolute magnitude of 5.93, so at a distance of 48 light years it has an apparent magnitude of 6.77 when viewed from earth. It also has a total Proper Motion of 0.210"/yr and belongs to the Ursa Major stream.
The system is a much studied BY Draconis variable star with a period of 6.99 days[4] The primary star has a spectral type of K3Vk. The secondary star in the system has a surface temperature of 4486±50 K and orbits the primary in about seven days.[8][9]
References
- Bopp, B. W.; Noah, P.; Klimke, A.; Hall, D. S.; Henry, G. W. (August 1981). "Photometry of HD 45088 : a new bright BY DRA variable". Publications of the Astronomical Society of the Pacific. 93: 504–506. doi:10.1086/130867. Retrieved 7 January 2022.
- Brown, A. G. A.; et al. (2016). "Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties". Astronomy and Astrophysics. 595. A2. arXiv:1609.04172. Bibcode:2016A&A...595A...2G. doi:10.1051/0004-6361/201629512. hdl:2445/125903. S2CID 1828208.Gaia Data Release 1 catalog entry
- Koen, C.; et al. (April 2010), "UBV(RI)C JHK observations of Hipparcos-selected nearby stars", Monthly Notices of the Royal Astronomical Society, 403 (4): 1949–1968, Bibcode:2010MNRAS.403.1949K, doi:10.1111/j.1365-2966.2009.16182.x.
- Bopp, B. W. (1980). "HD 45088 as a BY Draconis variable". Publications of the Astronomical Society of the Pacific. 92: 218–220. Bibcode:1980PASP...92..218B. doi:10.1086/130651.
- Glazunova, L. V.; et al. (2014). "Absolute parameters and chemical composition of the binary star OU Gem". Monthly Notices of the Royal Astronomical Society. 444 (2): 1901–1908. Bibcode:2014MNRAS.444.1901G. doi:10.1093/mnras/stu1576.
- Fuhrmann, Klaus (2008). "Nearby stars of the Galactic disc and halo - IV". Monthly Notices of the Royal Astronomical Society. 384 (1): 173–224. Bibcode:2008MNRAS.384..173F. doi:10.1111/j.1365-2966.2007.12671.x.
- "V* OU Gem". SIMBAD. Centre de données astronomiques de Strasbourg.
- "Aricns 4C00500".
- "Multiwavelength optical observations of chromospherically active bina…" (PDF). Archived from the original (PDF) on 2012-12-09.
External links
Constellation of Gemini |
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На других языках
- [en] OU Geminorum
[ru] OU Близнецов
OU Близнецов (лат. OU Geminorum, HD 45088) — кратная звезда в созвездии Близнецов на расстоянии приблизительно 48,2 световых лет (около 14,8 парсек) от Солнца. Видимая звёздная величина звезды — от +6,81m до +6,76m[8]. Возраст звезды определён как составляющий около 250 млн лет[9]*.
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