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searching for Cataclysmic variable star 17 found (65 total)

alternate case: cataclysmic variable star

DX Andromedae (580 words) [view diff] exact match in snippet view article find links to article

DX Andromedae (often abbreviated to DX And) is a cataclysmic variable star in the constellation Andromeda. It has a typical apparent visual magnitude
Z Apodis (375 words) [view diff] exact match in snippet view article find links to article
Although described in the General Catalogue of Variable Stars as a cataclysmic variable star, it appears that it is a pulsating variable star, and has been
V1017 Sagittarii (325 words) [view diff] exact match in snippet view article find links to article
V1017 Sagittarii is a cataclysmic variable star system in the constellation Sagittarius. It first erupted in 1919, reaching magnitude 7. Its other eruptions
Z Camelopardalis (418 words) [view diff] exact match in snippet view article find links to article
Z Camelopardalis (Z Cam) is a cataclysmic variable star system in the northern constellation of Camelopardalis. It has an apparent visual magnitude which
DP Leonis (479 words) [view diff] exact match in snippet view article find links to article
approximately 990 light-years from the Sun based on parallax. It is a cataclysmic variable star of the AM Herculis-type also known as polars. The system comprises
SS Ursae Minoris (254 words) [view diff] exact match in snippet view article find links to article
SS Ursae Minoris is a cataclysmic variable star system in the constellation Ursa Minor. It was discovered visually and by its X-ray emissions separately
TU 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-mass
WX Pyxidis (336 words) [view diff] exact match in snippet view article find links to article
WX Pyxidis is a cataclysmic variable star system in the constellation Pyxis. Its X-ray emissions were discovered in 1984, after which a visual correlate
GK Persei (908 words) [view diff] exact match in snippet view article find links to article
Aquilae 1918 to something resembling a typical dwarf nova-type cataclysmic variable star. Surrounding GK Persei is the Firework nebula, a nova remnant
RW Ursae Minoris (797 words) [view diff] exact match in snippet view article find links to article
RW Ursae Minoris (Nova Ursae Minoris 1956) is a cataclysmic variable star system that flared up as a nova in the constellation Ursa Minor in 1956. Although
RZ Leonis Minoris (971 words) [view diff] exact match in snippet view article find links to article
RZ Leonis Minoris is a cataclysmic variable star system in the northern constellation of Leo Minor. It undergoes frequent outbursts that vary in brightness
RR Pictoris (806 words) [view diff] exact match in snippet view article find links to article
RR Pictoris, also known as Nova Pictoris 1925, is a cataclysmic variable star system that flared up as a nova that lit up in the constellation Pictor
RX Andromedae (737 words) [view diff] exact match in snippet view article find links to article
Cataclysmic variable star system in the constellation Andromeda
RR Caeli (938 words) [view diff] exact match in snippet view article find links to article
approximately 9–20 billion years, RR Caeli will likely become a cataclysmic variable star due to the period's gradual shortening, leading to increasing
52 Europa (867 words) [view diff] exact match in snippet view article find links to article
the effort came up empty. It has been found that the reputed cataclysmic variable star CV Aquarii, discovered in 1934, was actually a misidentification
Mensa (constellation) (4,058 words) [view diff] exact match in snippet view article
magnitude of 8.05, it is 707 ± 6 light-years distant. AH Mensae is a cataclysmic variable star system composed of a white dwarf and a red dwarf that orbit each
Ursa Minor (5,853 words) [view diff] exact match in snippet view article find links to article
and transferring matter to the primary. RW Ursae Minoris is a cataclysmic variable star system that flared up as a nova in 1956, reaching magnitude 6