R Arae
Appearance
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Ara |
Right ascension | 16h 39m 44.7306s[1] |
Declination | −56° 59′ 39.867″[1] |
Apparent magnitude (V) | 6.65[1] |
Characteristics | |
Spectral type | B9IV/V[1] |
B−V color index | 0.09[1] |
Variable type | Algol[2] |
Astrometry | |
Proper motion (μ) | RA: -8.34[1] mas/yr Dec.: -18.85[1] mas/yr |
Parallax (π) | 8.06 ± 1.66 mas[1] |
Distance | approx. 400 ly (approx. 120 pc) |
Absolute magnitude (MV) | 1.18 |
Other designations | |
Database references | |
SIMBAD | data |
Data sources: | |
Hipparcos Catalogue, CCDM (2002), Bright Star Catalogue (5th rev. ed.) |
R Arae is an Algol-type eclipsing binary in the constellation Ara. Located approximately 124 parsecs (400 ly) distant,[1] it normally shines at magnitude 6.17, but during eclipses can fall as low as magnitude 7.32.[2] It has been suggested by multiple studies that mass transfer is occurring between the two stars of this system,[3][4] and the period of eclipses seems to be increasing over time.[4]
References
- ^ a b c d e f g h i "R Arae". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 30 June 2014.
- ^ a b VSX (25 October 2010). "R Arae". AAVSO Website. American Association of Variable Star Observers. Retrieved 30 June 2014.
- ^ Nield, K. M. (1991). "Observations and analysis of the Southern binary R Arae". Astrophysics and Space Science. 180 (2): 233. Bibcode:1991Ap&SS.180..233N. doi:10.1007/BF00648180.
- ^ a b Reed, P. A.; McCluskey Jr., G. E.; Kondo, Y.; Sahade, J.; Guinan, E. F.; GiméNez, A.; Caton, D. B.; Reichart, D. E.; Ivarsen, K. M.; Nysewander, M. C. (2010). "Ultraviolet study of the active interacting binary star R Arae using archivalIUEdata". Monthly Notices of the Royal Astronomical Society. 401 (2): 913. arXiv:0909.4047. Bibcode:2010MNRAS.401..913R. doi:10.1111/j.1365-2966.2009.15741.x.
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