RR Coronae Borealis explained
RR Coronae Borealis should not be confused with R Coronae Borealis.
RR Coronae Borealis (RR CrB, HD 140297, HIP 76844) is a M3-type semiregular variable star located in the constellation Corona Borealis with a parallax of 2.93mas being a distance of 341pc. It varies between magnitudes 7.3 and 8.2 over 60.8 days.[1] Located around 1228 light-years distant, it shines with a luminosity approximately 2180 times that of the Sun and has a surface temperature of 3309 K.[2]
Notes and References
- Web site: RR Coronae Borealis. Otero, Sebastian Alberto . 15 August 2011 . The International Variable Star Index. American Association of Variable Star Observers. 20 July 2014.
- McDonald, I.. Zijlstra, A. A.. Boyer, M. L.. 2012. Fundamental Parameters and Infrared Excesses of Hipparcos Stars. Monthly Notices of the Royal Astronomical Society. 427. 1. 343–57. 2012MNRAS.427..343M. 1208.2037 . 10.1111/j.1365-2966.2012.21873.x . 118665352.