YZ Cassiopeiae
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YZ Cassiopeiae (21 Cas) is a star system Script error: No such module "convert". away from Earth, in the constellation Cassiopeia. It comprises three stars: an eclipsing Algol-type binary and a visually fainter star about 3000 AU distant.[11] It is faintly visible to the naked eye under good observing conditions.
The primary star in the YZ Cassiopeiae system is a white subgiant (main sequence) star of spectral type A1Vm and 2.31 solar masses[11] (Template:Solar mass) with a less massive main sequence dwarf star of type F2V[3] and 1.35 Template:Solar mass.[11]
In 1924, Joel Stebbins announced his discovery that the star, then known as 21 Cassiopeiae, is an eclipsing binary.[16] It was given its variable star designation, YZ Cassiopeiae, in 1925.[17] The apparent magnitude of the eclipsing binary varies from 5.65 to 6.05[3] with a period of 4.4672 days.[11] Combined, they appear to have a spectral type of A2IV.[11]
The binary has a dimmer (magnitude 9.7 according to Norton,[18] or 10.5 by SIMBAD) companion of 0.8 Template:Solar mass[11] orbiting with a period of about 86 580 years.[11]
References
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- ↑ a b c d e Script error: No such module "Citation/CS1".
- ↑ a b c Jerzy M. Kreiner, Chun-Hwey Kim, Il-Seong Nha. YZ CAS: Atlas of O-C Diagrams of Eclipsing Binary Stars
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- ↑ a b c d e f g h Tokovinin 1997-1999. J/A+AS/124/75. Multiple star catalogue (MSC)
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- ↑ Template:Cite simbad
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- Triple star systems
- Eclipsing binaries
- Cassiopeia (constellation)
- A-type subgiants
- F-type main-sequence stars
- Flamsteed objects
- Objects with variable star designations
- Durchmusterung objects
- Henry Draper Catalogue objects
- Hipparcos objects
- Bright Star Catalogue objects