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3 cepheid variables
астр.• цефеидаEnglish-Bulgarian polytechnical dictionary > cepheid variables
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5 cepheid variable stars
estrellas variables cefeidasEnglish-Spanish dictionary of astronomy terms > cepheid variable stars
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переменная (звезда)@cataclysmic variableвзрывная переменная звезда@cepheid variableцефеида@early-type variablesпеременные ранних классов@eclipsing variableзатменная переменная звезда@galactic variableгалактическая переменная звезда@improver variableпсевдопеременная звезда@intrinsic variableистинная переменная звезда@irregular variablesнеправильные переменные@late-type variableпеременная звезда позднего класса@long-period variableдолгопериодическая переменная звезда@luminous blue variableяркая голубая переменная@magnetic variableмагнитная переменная@nebular variableпеременная звезда, связанная с туманностью@nonperiodic variableнеправильная переменная звезда@nova-like variableновоподобная переменная@occultation variableзатменная переменная звезда@physical variableфизическая переменная звезда@proper variableистинная переменная звезда@rapid variableкороткопериодическая переменная звезда@regular variableправильная переменная звезда@rotational variableвращающаяся переменная звезда@semiregular variableполуправильная переменная звезда@short-period variableкороткопериодическая переменная звезда@slow variableмедленная переменная звезда@spectral variableспектральная переменная@v/r variableпеременная с разделенными компонентами спектральных линий@
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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
cepheid — 1. adjective Relating to cepheid variables. 2. noun A cepheid variable … Wiktionary
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
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
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
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
RR Lyrae variable — RR Lyrae variables are periodic variable stars, commonly found in globular clusters, and often used as standard candles to measure galactic distances. This type of variable is named after the prototype, the variable star RR Lyrae in the… … Wikipedia
Large Magellanic Cloud — The Large Magellanic Cloud Observation data (J2000 epoch) Constellation Dorado/Mensa … Wikipedia
Delta Cephei — For the variable star type, see Delta Cephei variable. For the general type of variable star, see Cepheid variable. Alrediph, δ Cep A/B Location of δ Cephei (bottom left) … Wikipedia
