yellow supergiant
11Beta Aquarii — Starbox begin name=β Aquarii Starbox image caption = β Aquarii Starbox observe epoch=J2000 ra=21h 31m 33.5341s dec= 05° 34 prime; 16.22 Prime; appmag v=2.91 constell=Aquarius Starbox character class=G0Ib b v=0.83 u b=0.56 variable= Starbox… …
12RV Tauri — Starbox short name=RV Tauri epoch=J2000.0 constell=Taurus ra=4h 47m 6.7s dec=+26° 10 46 spectral=G2eIa M2Ia appmag v=9.8 ndash;13.3 dist ly=approx 20000 dist pc=approx 6000 names=HD 283868, BD+25 732RV Tauri is a star in the constellation Taurus …
13Beta Leporis — (β Lep / β Leporis) is a star in the constellation Lepus and is also known as NihalFact|date=October 2008. Beta Leporis has apparent magnitude +2.81 and is 159.2 light years from Earth. It is a yellow supergiant of spectral class G5II with 150… …
14Alpha Persei Cluster — Observation data (2000.0 epoch) Constellation Perseus …
15Cepheid (variable) — [sef′ē id, sē′fēid] n. 〚after CEPHEUS + ID〛 any of a class of pulsating, yellow, supergiant stars whose brightness varies in regular periods: from the period luminosity relation, the distance of such a star can be determi …
16Algenib — noun a) A yellow supergiant in the constellation Perseus; Alpha (α) Persei. b) A variable star in the constellation Pegasus; Gamma (γ) Pegasi. It forms one corner of the square of Pe …
17Mirfak — noun a yellow supergiant star in the constellation of Perseus Syn: Algenib …
18Cepheid Variable — A Yellow Supergiant star that changes its brightness in a rather accurate cycle. The brightness may change in a day, or it may take hundreds of days. The change in brightness is caused by the star expanding and contracting like a balloon. The… …
The writer's dictionary of science fiction, fantasy, horror and mythology
19Cepheid (variable) — [sef′ē id, sē′fēid] n. [after CEPHEUS + ID] any of a class of pulsating, yellow, supergiant stars whose brightness varies in regular periods: from the period luminosity relation, the distance of such a star can be determined: sometimes cepheid… …
20Cepheid (variable) — [sef′ē id, sē′fēid] n. [after CEPHEUS + ID] any of a class of pulsating, yellow, supergiant stars whose brightness varies in regular periods: from the period luminosity relation, the distance of such a star can be determined: sometimes cepheid… …
