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  2. Binary star - Wikipedia

    en.wikipedia.org/wiki/Binary_star

    From the orbital pattern of a visual binary, or the time variation of the spectrum of a spectroscopic binary, the mass of its stars can be determined, for example with the binary mass function. In this way, the relation between a star's appearance (temperature and radius) and its mass can be found, which allows for the determination of the mass ...

  3. Binary system - Wikipedia

    en.wikipedia.org/wiki/Binary_system

    (See animated examples.) The most common kinds of binary system are binary stars and binary asteroids, but brown dwarfs, planets, neutron stars, black holes and galaxies can also form binaries. A multiple system is similar but consists of three or more objects, for example triple stars and triple asteroids (a more common term than 'trinary').

  4. Category:Binary stars - Wikipedia

    en.wikipedia.org/wiki/Category:Binary_stars

    Pages in category "Binary stars" The following 200 pages are in this category, out of approximately 734 total. This list may not reflect recent changes.

  5. Star system - Wikipedia

    en.wikipedia.org/wiki/Star_system

    For example, the stars Gliese 644A and Gliese 644B form what appears to be a close visual binary star; because Gliese 644B is a spectroscopic binary, this is actually a triple system. The triple system has the more distant visual companion Gliese 643 and the still more distant visual companion Gliese 644C, which, because of their common motion ...

  6. List of brightest stars - Wikipedia

    en.wikipedia.org/wiki/List_of_brightest_stars

    For example, the binary star system Alpha Centauri has the total or combined magnitude of −0.27, while its two component stars have magnitudes of +0.01 and +1.33. [3] New or more accurate photometry, standard filters, or adopting differing methods using standard stars can measure stellar magnitudes slightly differently. This may change the ...

  7. O-type main-sequence star - Wikipedia

    en.wikipedia.org/wiki/O-type_main-sequence_star

    θ Muscae is a naked-eye Wolf-Rayet star, but the majority of the visible light is produced by an O-class main sequence companion and an OB supergiant. 9 Sagittarii is a spectroscopic binary containing O3.5 and O5–5.5 main sequence stars, making for the brightest star visible within the Lagoon Nebula. μ Columbae is a naked-eye O9.5 main ...

  8. Researchers find binary stars orbiting near Milky Way's ... - AOL

    www.aol.com/news/researchers-binary-stars...

    International researchers recently spotted a pair of stars orbiting around one another in surprisingly close proximity to Sagittarius A*. Researchers find binary stars orbiting near Milky Way's ...

  9. List of nearest stars by spectral type - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_stars_by...

    Below there are lists the nearest stars separated by spectral type.The scope of the list is still restricted to the main sequence spectral types: M, K, F, G, A, B and O.It may be later expanded to other types, such as S, D or C.