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Asymptotic giant branch stars stellar winds

Low- and intermediate-mass stars ultimately become asymptotic giant branch (AGB) stars and start to form dust in the cool stellar wind by which they eject their envelopes (see also Chapter 5). This dust is also mixed into the ISM like the returned gaseous material. About one half of the mass returned by AGB stars is... [Pg.36]

See other pages where Asymptotic giant branch stars stellar winds is mentioned: [Pg.140]    [Pg.29]    [Pg.275]    [Pg.171]    [Pg.16]    [Pg.191]    [Pg.68]    [Pg.35]    [Pg.307]    [Pg.81]    [Pg.115]    [Pg.362]    [Pg.132]    [Pg.647]   
See also in sourсe #XX -- [ Pg.147 ]



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Asymptotic giant branch stars

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Star-branched

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