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...

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...

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 shell star. VV...

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...

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...

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...

Beta Cephei variables, also known as Beta Canis Majoris stars, are variable stars that exhibit small rapid variations in their brightness due to pulsations...

ISSN 0004-6361. S2CID 17789027. "Mu Cephei | aavso". www.aavso.org. Retrieved 6 October 2024. Ramstedt, S.; Olofsson, H. (25 May 2014). "The 12CO/13CO ratio...

estimated mass of 1,937 M☉, of which about 24% is interstellar matter. A Delta Cephei type variable star designated U Sagittarii is a member of this cluster,...

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...

U Cephei is an eclipsing binary star discovered in 1880. It consists of a blue-white main sequence star of spectral type B7Ve that is eclipsed every two...

RW Cephei is a K-type hypergiant and a semirregular variable star in the constellation Cepheus, at the edge of the Sharpless 132 H II region and close...

SS Cephei is a variable star in the constellation Cepheus. It is of spectral type M5IIIvar, and has an estimated temperature of 3,700 °F (2,310 K). The...

Cephei ("Errai") by 3000 AD, with Errai reaching its closest alignment with the northern celestial pole around 4200 AD. Iota Cephei and Beta Cephei will...

consisting of η Cephei, 4 Cephei, HD 194298, θ Cephei, α Cephei, ξ Cephei, 26 Cephei, ι Cephei and ο Cephei. Consequently, the Chinese name for η Cephei itself...

rise to maximum light followed by a slower fall to minimum (e.g. Delta Cephei). This is due to the phase difference between the radius and temperature...

W Cephei is a spectroscopic binary and variable star located in the constellation Cepheus. It is thought to be a member of the Cep OB1 stellar association...

asterism consisting of Xi Cephei, 4 Cephei, HD 194298, Eta Cephei, Theta Cephei, Alpha Cephei, 26 Cephei, Iota Cephei and Omicron Cephei. Consequently, the Chinese...

Nu Cephei (ν Cephei) is a class A2, fourth-magnitude blue supergiant star in the constellation Cepheus, visible to the naked eye. It is a white pulsating...

Kappa Cephei, Latinized from κ Cephei, is a binary star system in the northern circumpolar constellation of Cepheus. It is visible to the naked eye as...

DH Cephei is a variable binary star system in the northern circumpolar constellation of Cepheus, positioned about two degrees to the east of the star system...

V Cephei is a white main sequence star in the constellation Cepheus. It only varies slightly by 0.03 of a magnitude. It was suspected of being variable...

helium is doubly ionized. The term Cepheid originates from the star Delta Cephei in the constellation Cepheus, which was one of the early discoveries. On...

Sciences 25th Annual Symposium on Telescope Science. Held May 23–25. 25: 47. Bibcode:2006SASS...25...47W. Otero, S. A.; Moon, T. (December 2006). "The Characteristic...

than other famous red supergiants such as Antares A, Betelgeuse, VV Cephei A, Mu Cephei, VY Canis Majoris, WOH G64, and UY Scuti. Nevertheless, its size...

Distance 317 ± 3 ly (97.1 ± 0.9 pc) Absolute magnitude (MV) 0.52 Details Mass 2.25? M☉ Radius 3.98+0.11 −0.13 R☉ Luminosity 44.3±0.5 L☉ Temperature 7466+217...

greater mass than the Sun: 107% and 105%, respectively. The system is about 2.25 billion years old. van Leeuwen, F. (2007). "Validation of the new Hipparcos...

the detection of pulsations, the Aa component has been classified as a β Cephei variable. Beta Centauri is well known in the Southern Hemisphere as the...

Population III stars. Such stars would dwarf VY Canis Majoris, Mu Cephei and VV Cephei A, three among the largest known modern stars. Once the black hole...

PV Cephei is a variable star of Orion type located in the constellation of Cepheus at a distance of about 1,100 light-years from Earth. In visible light...