- Mu
Cephei (Latinized from μ
Cephei,
abbreviated Mu Cep or μ Cep), also
known as the
Garnet Star, is a red
supergiant star in the
constellation Cepheus...
-
Gamma Cephei (γ
Cephei,
abbreviated Gamma Cep, γ Cep) is a
binary star
system approximately 45 light-years away in the
northern constellation of Cepheus...
- Tauri.
Examples of
eclipsing binaries are
Epsilon Aurigae (Almaaz), VV
Cephei, and V766
Centauri (HR 5171).
Angular diameter measurements can be inconsistent...
- hypergiant,
together with the red
supergiants Mu
Cephei, MY
Cephei, VV
Cephei, V381
Cephei, and V354
Cephei are
among the
largest stars known. In addition...
- VV
Cephei, also
known as HD 208816, is an
eclipsing binary star
system located in the
constellation Cepheus. It is both a B[e] star and s**** star. As...
-
asterism consisting of α
Cephei, 4
Cephei, HD 194298, Eta
Cephei,
Theta Cephei, Xi
Cephei, 26
Cephei, Iota
Cephei and
Omicron Cephei. Consequently, the Chinese...
-
Delta Cephei (δ Cep, δ
Cephei) is a
quadruple star
system located approximately 887 light-years away in the
northern constellation of Cepheus, the King...
- V354
Cephei is a red
supergiant star
located within the
Milky Way. It is an
irregular variable located over 13,000 light-years away from the Sun. It has...
- U
Cephei is an
eclipsing binary star
discovered in 1880. It
consists of a blue-white main
sequence star of
spectral type B7/8V that is
eclipsed every two...
- Beta
Cephei variables, also
known as Beta
Canis Majoris stars, are
variable stars that
exhibit small rapid variations in
their brightness due to pulsations...
