In astronomy, a semiregular variable star, a type of variable star, is a giant or supergiant of intermediate and late (cooler) spectral type showing considerable...
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of Variable Stars, both Mira variables and semiregular variables, particularly those of type SRa, were often considered as long period variables. At...
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This is a list of semiregular variable stars. Variability ranges are taken from the General Catalogue of Variable Stars (GCVS) where these are visual...
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is the brightest star in the constellation, and the semiregular variable star Y Lyncis is a target for amateur astronomers. Six star systems have been...
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giant star, BM Scorpii, which contrasts sharply with its blue neighbours in photographs. BM Scorpii, is classed as a semiregular variable star, its brightness...
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defined by ISO 217 Satanic ritual abuse SRa or SRA, a type of semiregular variable star Senior Airman (SrA), a US Air Force rank Septic Reserve Area,...
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Cephei is also known as Herschel's Garnet Star due to its deep red colour. It is a semiregular variable star with a minimum magnitude of 5.1 and a maximum...
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Variable Stars Star portal Lists of astronomical objects Lists of stars List of semiregular variable stars List of stars that have unusual dimming periods...
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V-band, and distances are from the Gaia DR2 star catalogue. Long period variable Semiregular variable star Mattei, Janet Akyuz (1997). "1997JAVSO..25....
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A variable star is a star whose brightness as seen from Earth (its apparent magnitude) changes systematically with time. This variation may be caused...
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M-type red supergiant star nearing the end of its life. It is the second brightest star in Orion, and is a semiregular variable star. It serves as the "right...
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Betelgeuse (redirect from Betelgeuse (star))
reddish, semiregular variable star whose apparent magnitude, varying between +0.0 and +1.6, has the widest range displayed by any first-magnitude star. Betelgeuse...
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Aries (constellation) (section Variable stars)
Mira variable star that ranges in magnitude from a minimum of 15.2 to a maximum of 7.2 with a period of 371.1 days. T Arietis is a semiregular variable star...
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AR Cephei (category Semiregular variable stars)
AR Cephei (AR Cep) is a variable star in the constellation Cepheus. It is classified as a semiregular star, and has a maximum apparent magnitude of +7...
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IBM operating systems Solid rocket booster SRb, a subtype of semiregular variable star Swedish Red-and-White or Svensk Röd och Vit Boskap, a breed of...
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NML Cygni (category Semiregular variable stars)
cool hypergiant star, VY Canis Majoris, and is also known as a heavily mass-losing OH/IR supergiant. It is also a semiregular variable star with a period...
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RS Cancri (category Semiregular variable stars)
3639 and HD 78712, is a star about 490 light years from the Earth in the constellation Cancer. It is a semiregular variable star, ranging in brightness...
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MY Cephei (category Semiregular variable stars)
open cluster NGC 7419 in the constellation of Cepheus. It is a semiregular variable star with a maximum brightness of magnitude 14.4 and a minimum of magnitude...
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R Lyrae (category Semiregular variable stars)
4th magnitude semiregular variable star in the constellation Lyra, approximately 350 light years away from Earth. It is a red giant star of the spectral...
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elements and its core is composed of carbon and oxygen. It is a semiregular variable star of the Mu Cephei type, whose apparent magnitude varies between...
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RW Cygni (category Semiregular variable stars)
RW Cygni is a semiregular variable star in the constellation Cygnus, about a degree east of 2nd magnitude γ Cygni. Its apparent magnitude varies between...
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V509 Cassiopeiae (category Semiregular variable stars)
to a peak of +4.6 and now around +5.3 and is classified as a semiregular variable star of type SRd. It is undergoing strong mass loss as part of its...
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S Persei (category Semiregular variable stars)
orbit of Jupiter. It is also a semiregular variable, a star whose variations are less regular than those of Mira variables. S Persei was named by German...
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star behaviour. Located near Alkes is the red-hued R Crateris, a semiregular variable star of type SRb and a spectral classification of M7. It ranges from...
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and lying around 290 light-years distant. It is classified as a semiregular variable star and its brightness varies from magnitude +4.75 to +4.93. Described...
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X Herculis (category Semiregular variable stars)
X Herculis is a star about 400 light years from the Earth in the constellation Hercules. It is a semiregular variable star, ranging in brightness from...
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distinct star systems in the constellation Orion: ο1 Orionis (4 Orionis), an M3S semiregular variable star ο2 Orionis (9 Orionis), a K2 giant star All of...
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Mirach (redirect from Mirach (star))
of this star has been one of the stable anchor points by which other stars are classified. It is suspected of being a semiregular variable star whose apparent...
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light-years (150 parsecs) distant from the Solar System. It is a semiregular variable star that varies between a maximum magnitude of 6.14 and minimum magnitude...
43 KB (4,939 words) - 13:51, 2 September 2024