Long Secondary Periods in Pulsating Asymptotic Giant Branch Stars: An Investigation of their Origin
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
Collections | ANU Research Publications |
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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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