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Long Secondary Periods in Pulsating Asymptotic Giant Branch Stars: An Investigation of their Origin

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Wood, Peter R; Olivier, Enrico A; Kawaler, S D

Description

Approximately 25%-30% of pulsating asymptotic giant branch (AGB) stars show long secondary periods (LSPs) of typical length ∼400-1500 days, roughly 10 times longer than the primary period of pulsation. Here we seek an explanation for the LSPs. We descri

CollectionsANU Research Publications
Date published: 2004
Type: Journal article
URI: http://hdl.handle.net/1885/80820
Source: Astrophysical Journal, The
DOI: 10.1086/382123

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