-
orange hypergiant,
together with the red
supergiants Mu
Cephei, MY
Cephei, VV
Cephei, and V354
Cephei are
among the
largest stars known. In addition, Cepheus...
- VV
Cephei, also
known as HD 208816, is an
eclipsing binary star
system located in the
constellation Cepheus,
approximately 5,000
light years from Earth...
- Mu
Cephei (Latinized from μ
Cephei,
abbreviated Mu Cep or μ Cep), also
known as Herschel's
Garnet Star, Erakis, or HD 206936, is a red
supergiant or hypergiant...
-
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...
-
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...
-
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...
-
Scorpii A).
Examples of
eclipsing binaries are
Epsilon Aurigae (Almaaz), VV
Cephei, and V766
Centauri (HR 5171).
Angular diameter measurements can be inconsistent...
- V354
Cephei is a red
supergiant star
located within the
Milky Way. It is an
irregular variable located over 8,900 light-years away from the Sun. It has...
- The
Bayer designation Rho
Cephei (ρ
Cephei / ρ Cep) is
shared by two
stars in the
constellation Cepheus: ρ1
Cephei ρ2
Cephei This
article includes a list...
- Beta
Cephei (β
Cephei,
abbreviated Beta Cep, β Cep) is a
triple star
system of the
third magnitude in the
constellation of Cepheus.
Based on
parallax measurements...
