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Two Different Stellar Populations in the Large Magellanic Cloud?

Published online by Cambridge University Press:  07 August 2017

JU. Frantsman  and
I. Shmeld
JU. Frantsman
Affiliation:
Radioastrophysical observatory, Latvian Acad. Sci., Turgeneva 19, Riga, LV-1527 LATVIA
I. Shmeld
Affiliation:
Radioastrophysical observatory, Latvian Acad. Sci., Turgeneva 19, Riga, LV-1527 LATVIA

Extract

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The evolution of stars on the AGB has been explained as episodic helium burning and neutron capture nucleosynthesis in the stellar interior, followed by the mixing of a portion of the processed material into the envelope of a star. The simple stellar evolutionary scheme M–MS–S–SC–N had been accepted. However in recent years extensive observations of AGB stars have shown that evolution of the AGB is more complicated than painted in such a simple picture.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 164: Stellar Populations , 1995 , pp. 415
Copyright
Copyright © Kluwer 1995