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1 цефеида
Cepheid variableцефеиды с биениями3 beat Cepheidsцефеиды типа RR Лиры1.RR Lyrae stars 2.cluster variables 3.short-period Cepheidsкарликовая цефеида1.dwarf Cepheid (δ Scuto star) 2.Scuti starмолодые цефеиды дискаyoung disk Cepheidsультракороткопериодические цефеидыultrashort-period Cepheids -
2 долгопериодические цефеиды
Makarov: classical cepheids, long-period cepheidsУниверсальный русско-английский словарь > долгопериодические цефеиды
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3 долгопериодические цефеиды
long-period cepheids, classical cepheidsРусско-английский физический словарь > долгопериодические цефеиды
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4 карликовые цефеиды
Makarov: dwarf cepheidsУниверсальный русско-английский словарь > карликовые цефеиды
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5 классические цефеиды
Makarov: classical cepheidsУниверсальный русско-английский словарь > классические цефеиды
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6 короткопериодические цефеиды
Makarov: short-period cepheidsУниверсальный русско-английский словарь > короткопериодические цефеиды
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7 цефеиды
1) Astronomy: cepheids2) Makarov: cepheid variables, cepheides -
8 карликовые цефеиды
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9 классические цефеиды
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10 короткопериодические цефеиды
Русско-английский физический словарь > короткопериодические цефеиды
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11 цефеиды
мн.; астр.cepheids; cepheid variables- карликовые цефеиды
- классические цефеиды
- короткопериодические цефеиды -
12 биения
beat (for cepheids)
См. также в других словарях:
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
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
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
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
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
Cepheid variable — Astron. a variable star in which changes in brightness are due to alternate contractions and expansions in volume. Also, cepheid variable. [1900 05; CEPHE(US) + ID1] * * * One of a class of variable stars whose period of variation is closely… … Universalium
Large Magellanic Cloud — The Large Magellanic Cloud Observation data (J2000 epoch) Constellation Dorado/Mensa … 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
Baade , Wilhelm Heinrich Walter — (1893–1960) German–American astronomer Baade, born the son of a schoolteacher in Schröttinghausen, Germany, was educated at the universities of Münster and Göttingen, where he obtained his PhD in 1919. He worked at the University of Hamburg s… … Scientists