Identification of oxygen-rich evolved stars by maser surveys and statistical studies on infrared data

The post-asymptotic giant branch (post-AGB) phase is a short episode in the life of a star with mass between 0.8 to 8 M⊙. It comes after the AGB phase, and before the planetary nebula phase. A rapid change in many physical properties of a star is suggested to happen in this phase, for example the on...

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Bibliographic Details
Main Authors: Yung, Hong-kiu, Bosco, 容康喬
Other Authors: Kwok, S
Language:English
Published: The University of Hong Kong (Pokfulam, Hong Kong) 2014
Subjects:
Online Access:http://hdl.handle.net/10722/193506