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Variable star - Wikipedia, the free encyclopedia
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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 a...
en.wikipedia.org/wiki/Variable_star
Binary star - Wikipedia, the free encyclopedia
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A binary star is a star system consisting of two stars orbiting around their common center of mass. The brighter star is called the primary and the other is its companion star , comes , or se...
en.wikipedia.org/wiki/Binary_star
Encyclopedia article about eclipsing variable star. Information about eclipsing variable star in the Columbia Encyclopedia, Computer Desktop Encyclopedia, computing dictionary. ... Eclipsing binaries; eclipsing binary; eclipsing binary; eclipsing binary; eclipsing binary; Eclipsing binary star; Eclipsing binary star;
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In addition, these close double stars are useful in studies of mass loss and of stellar evolution. Since eclipsing stars are variable in light, they are included in general variable star catalogs under the same system of nomenclature.
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Search Results: Eclipsing variable stars ... Double star systems in which the two components are too close to be seen separately but which reveal their duplicity by periodic changes in...
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Hutchinson encyclopedia article about eclipsing variable star. eclipsing variable star. Information about eclipsing variable star in the Hutchinson encyclopedia. ... (redirected from eclipsing variable star)
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Another type is the eclipsing binary, a double star in which the two stars periodically pass in front of each other as seen from Earth. When one star crosses in front of ... Eclipsing binary star; eclipsing variable star; eclipsing variable star; eclipsing variable star; eclipsis; eclipsis; eclipsis; eclipsis; Eclipso;
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Sky & Telescope, the Essential Magazine of Astronomy. News, observing tips, how-to advice, and more! ... Now you can calculate the dates and times (local and Universal Times) when the eclipsing variable star Algol should be at its dimmest (magnitude 3.4 instead of its usual 2.1).
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stars: binaries: eclipsing, starspots, stars: individual: RU UMi; 1. Introduction; RU Ursae Minoris (BD+700751) was discovered as an eclipsing variable star by Strohmeier & Knigge (1960). After its discovery, numerous observations of the system have been made by various observers.
www.aanda.org/articles/aa/pdf/2001/15/aa10540.pdf
American Association of Variable Star Observers (Popularity: ): The largest organization for variable stars: provides professional and amateur collaboration, research, and analysis of ... ... Astronomical Society of South Australia (Popularity: ): ASSA's variable star group. News, FAQ, charts, and software.
www.sciencecentral.com/site/510440