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CENTER OF MASS: The common point around which two stars in a binary system orbit.

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ORBITAL PERIOD: The time it takes for two stars in a binary system to complete one orbit around their common center of mass.

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ECLIPSING BINARY: A binary star system in which one star periodically passes in front of the other, causing periodic dimming.

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SPECTROSCOPIC BINARY: A binary star system where the stars cannot be resolved visually, but their orbital motion can be detected through shifts in spectral lines.

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VISUAL BINARY: A binary star system in which the two stars can be individually observed with a telescope.

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BINARY STAR SYSTEM: A system containing two stars that are gravitationally bound and orbit a common center of mass.

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BINARY AND MULTIPLE STAR SYSTEMS

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NOVA: An explosive event in a binary system involving a white dwarf accreting material from a companion star, leading to a sudden increase in brightness.

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ACCRETION IN WHITE DWARFS: A white dwarf can gain mass from a companion star in a binary system, possibly leading to nova explosions.

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MAGNETIC ACTIVITY IN WHITE DWARFS: Some white dwarfs exhibit strong magnetic fields, which can influence their surrounding environment.