Long Secondary Periods in Pulsating Asymptotic Giant Branch Stars: An Investigation of their Origin
Loading...
Date
Authors
Wood, Peter R
Olivier, Enrico A
Kawaler, S D
Journal Title
Journal ISSN
Volume Title
Publisher
IOP Publishing
Abstract
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
Description
Citation
Collections
Source
Astrophysical Journal, The