dwarf cepheids

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• Dwarf nova — HT Cas seen in outburst (mag 13.4) on 2010 November 2. Li …   Wikipedia

• Pulsating white dwarf — V777 Herculis star redirects here. For the star, see GD 358. A pulsating white dwarf is a white dwarf star whose luminosity varies due to non radial gravity wave pulsations within itself. Known types of pulsating white dwarfs include DAV, or ZZ… …   Wikipedia

• Variable star — A star is classified as variable if its apparent brightness as seen from Earth changes over time, whether the changes are due to variations in the star s actual luminosity, or to variations in the amount of the star s light that is blocked from… …   Wikipedia

• Cepheid variable — This article is about a class of pulsating stars. For the similarly named constellation, see Cepheus (constellation). Cepheids redirects here. For the fictional species, see Blind Alley . A Cepheid (  /ˈs …   Wikipedia

• Переменные типа SX Феникса — (SXPHE) тип переменных звёзд, показывающих краткие периодические пульсации с переменной амплитудой изменения блеска, которая может достигать 0.7m на временных масштабах 0.03 0.08 дней (0.7 1.9 часа)[1]. Они являются пульсирующими субкарликами… …   Википедия

• Переменная типа SX Феникса — Переменные типа SX Феникса (SXPHE)  тип переменных звёзд, показывающих краткие периодические пульсации с переменной амплитудой изменения блеска, которая может достигать 0.7m на временных масштабах 0,03 0,08 дней (0,7 1,9 часа)[1]. Они… …   Википедия

• star — starless, adj. /stahr/, n., adj., v., starred, starring. n. 1. any of the heavenly bodies, except the moon, appearing as fixed luminous points in the sky at night. 2. Astron. any of the large, self luminous, heavenly bodies, as the sun, Polaris,… …   Universalium

• galaxy — /gal euhk see/, n., pl. galaxies. 1. Astron. a. a large system of stars held together by mutual gravitation and isolated from similar systems by vast regions of space. b. (usually cap.) See Milky Way. 2. any large and brilliant or impressive… …   Universalium

• Cosmic distance ladder — * Light green boxes: Technique applicable to star forming galaxies. * Light blue boxes: Technique applicable to Population II galaxies. * Light Purple boxes: Geometric distance technique. * Light Red box: The planetary nebula luminosity function… …   Wikipedia

• Classical Cepheid variable — Classical Cepheids (also known as Population I Cepheids, Type I Cepheids, or Delta Cephei variables) are a type of Cepheid variable star. They are population I, variable stars that exhibit pulsation periods in the order of a few days to months,… …   Wikipedia

• Type II Cepheid — Type II Cepheids are variable stars which pulsate with periods typically between 1 and 50 days.[1][2] Type II Cepheids are population II stars and are thus old, typically metal poor, low mass objects.[1] Type II Cepheids were historically called… …   Wikipedia