Astronomy:S Coronae Australis

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Short description: Variable star in the constellation Corona Australis
S Coronae Australis
SCrALightCurve.png
A visual band light curve for S Coronae Australis, adapted from Mundt (1979).[1] The error bar shown on the left-most point applies to all points.
Observation data
Equinox J2000.0]] (ICRS)
Constellation Corona Australis
Right ascension {{{ra}}}
Declination −36° 57′ 19.8950″[2]
Apparent magnitude (V) 10.91[2]
Characteristics
Spectral type G0Ve + K0Ve[3]
Variable type T Tau[3]
Astrometry
Radial velocity (Rv)−33 ± 5[4] km/s
Proper motion (μ) RA: −2.6 ± 5.8[2] mas/yr
Dec.: −9.8 ± 2.3[2] mas/yr
Distance460 ly
(140[3] pc)
Details
Other designations
S CrA, S Coronae Australis, HH 82
Database references
SIMBADdata

S Coronae Australis (S CrA), is a young binary star system estimated to be around 2 million years old located in the constellation Corona Australis. It is composed of a G-type main sequence star that is about as luminous as and just over twice as massive as the Sun, and a smaller K-type main sequence star that has around 50-60% of the Sun's luminosity and 1.3 times its mass. Both stars are T Tauri stars and both show evidence of having circumstellar disks. The system is around 140 parsecs distant.[3]

References

  1. Mundt, R. (April 1979). "Spectroscopic and photometric variations of the YY Orionis star S CrA". Astronomy & Astrophysics 74: 21–29. Bibcode1979A&A....74...21M. https://ui.adsabs.harvard.edu/abs/1979A&A....74...21M. Retrieved 14 December 2021. 
  2. 2.0 2.1 2.2 2.3 Cite error: Invalid <ref> tag; no text was provided for refs named UCAC4
  3. 3.0 3.1 3.2 3.3 Carmona, A.; van den Ancker, M. E.; Henning, Th. (2007). "Optical spectroscopy of close companions to nearby Herbig Ae/Be and T Tauri stars". Astronomy and Astrophysics 464 (2): 687–95. doi:10.1051/0004-6361:20065509. Bibcode2007A&A...464..687C. 
  4. Ralph Elmer Wilson (1953). "General Catalogue of Stellar Radial Velocities". Carnegie Institute Washington D.C. Publication (Carnegie Institution of Washington). Bibcode1953GCRV..C......0W.