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| a loose group of young stars whose spectral types, motions, and positions in the sky indicate a common origin |
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| one of about 150 large, spherical star clusters (each with hundreds of thousands of stars) that form a spherical halo around the center of our Galaxy |
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| a nearly explosive ignition of helium in the triple-alpha process in the dense core of a red giant star |
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| location in the H–R diagram where stars begin to leave the main sequence |
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| the building up of heavy elements from lighter ones by nuclear fusion |
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| a comparatively loose cluster of stars, containing from a few dozen to a few thousand members, located in the spiral arms or disk of our Galaxy; sometimes referred to as a galactic cluster |
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| a shell of gas ejected by and expanding away from an extremely hot low-mass star that is nearing the end of its life (the nebulae glow because of the ultra-violet energy of the central star) |
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| a nuclear reaction by which three helium nuclei are built up (fused) into one carbon nucleus |
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| a line denoting the main sequence on the H–R diagram for a system of stars that have completed their contraction from interstellar matter and are now deriving all their energy from nuclear reactions, but whose chemical composition has not yet been altered substantially by nuclear reactions |
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