asymptotic giant branch oor Masedonies

asymptotic giant branch

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The region of the Hertzsprung-Russell diagram populated by evolving low to medium-mass stars.

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асимптотична џиновска гранка

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stars powered by fusion of hydrogen and helium in shell with an inactive core of carbon and oxygen
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Germanium is created by stellar nucleosynthesis, mostly by the s-process in asymptotic giant branch stars.
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For the more massive asymptotic giant branch stars that form planetary nebulae, whose progenitors exceed about 3M⊙, their cores will continue to contract.
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In red giant stars, and particularly during the asymptotic giant branch phase, the surface convection zone varies in depth during the phases of shell burning.
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A protoplanetary nebula (PPN) is an astronomical object at the short-lived episode during a star's rapid stellar evolution between the late asymptotic giant branch (LAGB) phase and the following planetary nebula (PN) phase.
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After a star passes through the asymptotic giant branch (AGB) phase, the short planetary nebula phase of stellar evolution begins as gases blow away from the central star at speeds of a few kilometers per second.
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During the late asymptotic giant branch (LAGB) phase, when mass loss reduces the hydrogen envelope's mass to around 10−2 M☉ for a core mass of 0.60 M☉, a star will begin to evolve towards the blue side of the Hertzsprung–Russell diagram.
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6 sinne gevind in 2 ms. Hulle kom uit baie bronne en word nie nagegaan nie.