Astronomy:OU Geminorum

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Short description: Multiple star system in the constellation Gemini
OU Geminorum
OUGemLightCurve.png
A visual band light curve for OU Geminorum, adapted from Bopp et al. (1981)[1]
Observation data
Equinox J2000.0]] (ICRS)
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
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[2] mas
Distance47.6 ± 0.2 ly
(14.61 ± 0.07 pc)
Absolute magnitude (MV)5.93±0.05[3]
Orbit[5]
PrimaryOU Gem Aa
CompanionOU 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]
OU Gem Aa
Mass0.85 M
Radius0.81 R
Surface gravity (log g)4.55 cgs
Temperature4960 K
OU Gem Ab
Mass0.71 M
Radius0.65 R
Surface gravity (log g)4.65 cgs
Temperature4390 K
Other designations
OU Gem, BD+18 1214, GJ 233, HD 45088, HIP 30630, SAO 95677[7]
Database references
SIMBADdata

OU Geminorum (OU Gem) is a visual binary or possible triple star located in the constellation of Gemini.

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

  1. 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. Bibcode1981PASP...93..504B. 
  2. 2.0 2.1 2.2 2.3 2.4 Brown, A. G. A. et al. (2016). "Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties". Astronomy and Astrophysics 595: A2. doi:10.1051/0004-6361/201629512. Bibcode2016A&A...595A...2G. Gaia Data Release 1 catalog entry
  3. 3.0 3.1 3.2 3.3 3.4 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. doi:10.1111/j.1365-2966.2009.16182.x. Bibcode2010MNRAS.403.1949K. 
  4. 4.0 4.1 Bopp, B. W. (1980). "HD 45088 as a BY Draconis variable". Publications of the Astronomical Society of the Pacific 92: 218–220. doi:10.1086/130651. Bibcode1980PASP...92..218B. 
  5. 5.0 5.1 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. doi:10.1093/mnras/stu1576. Bibcode2014MNRAS.444.1901G. 
  6. Fuhrmann, Klaus (2008). "Nearby stars of the Galactic disc and halo - IV". Monthly Notices of the Royal Astronomical Society 384 (1): 173–224. doi:10.1111/j.1365-2966.2007.12671.x. Bibcode2008MNRAS.384..173F. 
  7. "V* OU Gem". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=V%2A+OU+Gem. 
  8. "Aricns 4C00500". http://www.ari.uni-heidelberg.de/datenbanken/aricns/cnspages/4c00500.htm. 
  9. "Multiwavelength optical observations of chromospherically active bina…". http://cdsweb.cern.ch/record/411408/files/9912160.pdf. 

External links