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Find link is a tool written by Edward Betts.searching for SU Ursae Majoris 19 found (27 total)
alternate case: sU Ursae Majoris
SS Ursae Minoris
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understood to be coming from the same object. It is classified as a SU Ursae Majoris variable subclass of dwarf nova in that it has both 'normal' outburstsTV Corvi (640 words) [view diff] exact match in snippet view article find links to article
TV Corvi, also known as Tombaugh's Star, is a dwarf nova of the SU Ursae Majoris type in the constellation Corvus that was first discovered by accidentTU Mensae (359 words) [view diff] exact match in snippet view article find links to article
TU Mensae is a cataclysmic variable star of (SU Ursae Majoris subtype) in the constellation Mensa. A close binary, it consists of a white dwarf and low-massVW Hydri (233 words) [view diff] exact match in snippet view article find links to article
VW Hydri is a dwarf nova of the SU Ursae Majoris type in the deep southern constellation Hydrus; a star system that consists of a white dwarf and anotherEK Trianguli Australis (711 words) [view diff] exact match in snippet view article find links to article
in the constellation Triangulum Australe. It is a dwarf nova of the SU Ursae Majoris type that officially classified as such in 1980, after the characteristicSX Leonis Minoris (420 words) [view diff] exact match in snippet view article find links to article
SX Leonis Minoris is a dwarf nova of the SU Ursae Majoris type that was first discovered as a 16th magnitude blue star in 1957, before its identity wasRZ Leonis Minoris (971 words) [view diff] exact match in snippet view article find links to article
showing superoutbursts and superhumps. This indicates that RZ LMi is a SU Ursae Majoris-type dwarf novae belonging to the ER UMa sub-class. None of the variationWZ Sagittae (896 words) [view diff] exact match in snippet view article find links to article
reaching a photographic magnitude of 7.0. This nova is classified as a SU Ursae Majoris class star, which is a subclass of dwarf nova that produces what areTriangulum Australe (3,330 words) [view diff] exact match in snippet view article find links to article
Period of the SU Ursae Majoris Star EK Trianguli Australis and Evidence for Ring-Like Accretion Disks in Long-Supercycle Length SU Ursae Majoris Stars", PublicationsList of stars in Triangulum Australe (224 words) [view diff] exact match in snippet view article find links to article
Wolf–Rayet star, ΔV = 0.13m EK TrA EK 15h 14m 01.47s −65° 05′ 32.1″ 10.40 SU Ursae Majoris variable, Vmax = 10.4m, Vmin = <15.0m, P = 0.06288 d HD 141969 MM 141969YZ Leonis Minoris (1,422 words) [view diff] exact match in snippet view article find links to article
Association of Variable Star Observers also mentions YZ Leonis Minoris as a SU Ursae Majoris-type star (dwarf nova). YZ Leonis Minoris was the first system discoveredList of stars in Sagitta (75 words) [view diff] exact match in snippet view article find links to article
11.04m, Vmin = 11.12m RZ Sge RZ 20h 03m 18.47s +17° 02′ 51.9″ 12.3 SU Ursae Majoris variable, Vmax = 12.3m, Vmin = 17.7m, P = 0.0682803 d QY Sge QY 20hCataclysmic variable star (961 words) [view diff] exact match in snippet view article find links to article
stars Temporarily "halt" at a particular brightness below their peak SU Ursae Majoris stars Have "superoutbursts" which are brighter than the average SSHydrus (3,095 words) [view diff] exact match in snippet view article find links to article
Located 3° northeast of Gamma is the VW Hydri, a dwarf nova of the SU Ursae Majoris type. It is a close binary system that consists of a white dwarf andLeo Minor (3,840 words) [view diff] exact match in snippet view article find links to article
most stable celestial clock. SX Leonis Minoris is a dwarf nova of the SU Ursae Majoris type that was identified in 1994. It consists of a white dwarf andPlanet Hunters (3,510 words) [view diff] exact match in snippet view article find links to article
cataclysmic variable KIC 9406652. In April 2014 the unusually active SU Ursae Majoris-type dwarf nova GALEX J194419.33+491257.0 was discovered. This cataclysmicComa Berenices (6,955 words) [view diff] exact match in snippet view article find links to article
Comae Berenices. A June 2003 outburst from GO Comae Berenices, an SU Ursae Majoris-type dwarf nova, was photometrically observed. Coma Berenices has sevenVariable star (6,468 words) [view diff] exact match in snippet view article find links to article
standstills are seen, part way between maximum and minimum brightness. SU Ursae Majoris stars, which undergo both frequent small outbursts, and rarer but largerLyra (7,533 words) [view diff] exact match in snippet view article find links to article
still not fully understood. Another outbursting star is AY Lyrae, an SU Ursae Majoris-type dwarf nova that has undergone several superoutbursts. Of the same