RS Ophiuchi (RS Oph) is a recurrent nova system approximately 5,000 light-years away in the constellation Ophiuchus. In its quiet phase it has an apparent...

system with the primary being more massive and luminous than the Sun. RS Ophiuchi is part of a class called recurrent novae, whose brightness increase...

flaring is observed, the object is called a recurrent nova. An example is RS Ophiuchi, which is known to have flared seven times (in 1898, 1933, 1958, 1967...

85365 17h 26m 37.94s −05° 05′ 11.4″ 4.53 2.14 98 F3V Often mislabeled 47 Ophiuchi, which is in Serpens ρ Oph A ρ 5 13 147933 80473 16h 25m 35.12s −23° 26′ 49...

36 Ophiuchi (or Guniibuu for component A) is a triple star system 19.5 light-years from Earth. It is in the constellation Ophiuchus. The primary and secondary...

example of such a star system is RS Ophiuchi, a binary system consisting of a red giant and a white dwarf companion. RS Ophiuchi has flared into a (recurrent)...

(2008-12-19). "Recurrent Novae as a Progenitor System of Type Ia Supernovae. I. RS Ophiuchi Subclass: Systems with a Red Giant Companion - Abstract - The Astrophysical...

2020". www.aavso.org. "Alert Notice 752: Rare Outburst of Recurrent Nova RS Ophiuchi". www.aavso.org. Drake, Jeremy J.; Ness, Jan-Uwe; Page, Kim L.; Luna...

magnitudes, repeating every 10 to 80 years. Examples include T Pyxidis and RS Ophiuchi. Dwarf novae Dwarf novae, or U Geminorum stars, are cataclysmic variables...

Supernovae". In Evans, A.; Bode, M.F.; O'Brien, T.J.; Darnley, M.J. (eds.). RS Ophiuchi (2006) and the Recurrent Nova Phenomenon. ASP Conference Series. Vol...

70 Ophiuchi is a binary star system located 16.6 light years away from the Earth. It is in the constellation Ophiuchus. At magnitude 4 it appears as a...

explode with an hourglass shape already a few days after outburst (e.g. RS Ophiuchi), or the detection of disks in the heart of planetary nebulae. The Laboratoire...

UB313 is found to be larger than Pluto. February 13 – The recurrent nova RS Ophiuchi erupts. The last outburst occurred in 1985. March 9 – NASA's Cassini-Huygens...

Moores University Thesis A model for the remnant of the recurrent nova RS Ophiuchi (1985) (1990) Doctoral advisor Franz Daniel Kahn Website proftimobrien...

Timothy John (1990). A model for the remnant of the recurrent nova RS Ophiuchi (1985) (PhD thesis). University of Manchester. "Index entry". FreeBMD...

companion. It erupted in 1928 and 1996 and reached about magnitude 13. RS Ophiuchi HR Lyrae V838 Monocerotis Nogami, D.; et al. (2003). "The SU UMa Nature...

Scorpii by Gould, Theta Telescopii reverted to its old appellation of d Ophiuchi, and Sigma Telescopii was placed in Corona Australis. Initially uncatalogued...

dwarf C 70 Ophiuchi (16.7074±0.0087 ly) K-type main-sequence star B Gliese 570 (19.1987±0.0074 ly) 2 red dwarfs: B, C T-type brown dwarf D 36 Ophiuchi (19.4185±0...

L/Teff Another study give a much smaller radius of 555+55 −46 R☉. V1111 Ophiuchi (IRC +10365) 902 L/Teff RW Cephei 900–1,760, 940 L/Teff & AD A K-type hypergiant...

431+60 −47 [22] U Cygni 5.9 12.1 463 767+34 −31 [23] X Ophiuchi 5.9 8.6 338 215+15 −13 [24] RS Scorpii 6.0 13.0 319 709+306 −164 [25] RT Sagittarii 6...

Prominence Eruption Leading to a CME Associated with a Superflare on the RS CVn-type Star V1355 Orionis". The Astrophysical Journal. 948 (1): 9. arXiv:2301...

Gatewood, George (2005-08-01). "An Astrometric Study of the Binary Star α Ophiuchi". The Astronomical Journal. 130 (2): 809–814. Bibcode:2005AJ....130..809G...

Smith, Paul S. (2003). "The Newly Active R Coronae Borealis Star, V2552 Ophiuchi". The Publications of the Astronomical Society of the Pacific. 115 (813):...

The runaway star Zeta Ophiuchi and the bow shock formed by this massive star Puppis A, which is a supernova remnant The Rho Ophiuchi cloud complex Lambda...

of roughly 900 light years. It is located in the proximity of the Rho Ophiuchi dark cloud. This is a white A-type bright giant with a stellar classification...

Gliese 268 (QY Aurigae) is a RS Canum Venaticorum variable (RS CVn) star in the Auriga constellation. RS CVn variables are binary star systems with a...