SX Corvi

SX Corvi
	; A light curve for SX Corvi, plotted from Hipparcos data[1]
Observation data; Epoch J2000.0 Equinox J2000.0
Constellation	Corvus
Right ascension	12h 40m 15.04406s[2]
Declination	−18° 48′ 00.9336″[2]
Apparent magnitude (V)	8.99 - 9.25 [3]
Characteristics
Spectral type	F7V[3]
Variable type	W UMa
Astrometry
Radial velocity (Rv)	8.71 ± 0.94 km/s
Proper motion (μ)	RA: 39.16 ± 1.21 mas/yr ; Dec.: -6.07 ± 0.80 mas/yr
Parallax (π)	10.94 ± 1.18 mas[4]
Distance	approx. 300 ly ; (approx. 91 pc)
Details
Age	7.32 ± 0.97[5] Gyr
Other designations
	SX Corvi, HD 110139, HIP 61825, SAO 157434
Database references
SIMBAD	data

SX Corvi is an eclipsing binary star system in the constellation Corvus, ranging from apparent magnitude 8.99 to 9.25 over 7.6 hours.[3] The system is a contact binary also known as a W Ursae Majoris variable, where the two component stars orbit closely enough to each other for mass to have been transferred between them—in this case the secondary having transferred a large amount of mass to the primary.[5]

Yildiz and colleagues estimated the age of the system at 7.32 ± 0.97 billion years based on study of the properties of the system and estimated rate of mass transfer. They found the current masses of the primary and secondary to be 1.25 ± 0.04 and 0.10 ± 0.01 solar masses respectively, from their original masses of 0.72 ± 0.02 and 1.68 ± 0.05 solar masses.[5]

References

"Light Curve". Hipparcos ESA. ESA. Retrieved 17 February 2022.
"SX Crv -- Eclipsing binary of W UMa type (contact binary)". Retrieved 21 July 2015.
Watson, Christopher (19 April 2012). "SX Corvi". The International Variable Star Index. American Association of Variable Star Observers. Retrieved 21 July 2015.
van Leeuwen, F. (2007). "Validation of the New Hipparcos Reduction". Astronomy and Astrophysics. 474 (2): 653–64. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600.
Yildiz (2014). "Origin of W UMa-type contact binaries - age and orbital evolution". Monthly Notices of the Royal Astronomical Society. 437 (1): 185–94. arXiv:1310.5526. Bibcode:2014MNRAS.437..185Y. doi:10.1093/mnras/stt1874.

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[HIPCurve-1] "Light Curve". Hipparcos ESA. ESA. Retrieved 17 February 2022.

[SIMBAD-2] "SX Crv -- Eclipsing binary of W UMa type (contact binary)". Retrieved 21 July 2015.

[AAVSOSX-3] Watson, Christopher (19 April 2012). "SX Corvi". The International Variable Star Index. American Association of Variable Star Observers. Retrieved 21 July 2015.

[vanLeeuwen2007-4] van Leeuwen, F. (2007). "Validation of the New Hipparcos Reduction". Astronomy and Astrophysics. 474 (2): 653–64. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600.

[Yildiz-5] Yildiz (2014). "Origin of W UMa-type contact binaries - age and orbital evolution". Monthly Notices of the Royal Astronomical Society. 437 (1): 185–94. arXiv:1310.5526. Bibcode:2014MNRAS.437..185Y. doi:10.1093/mnras/stt1874.