Skip navigation
Skip navigation
The system will be down for maintenance between 8:00 and 8:15am on Thursday 13, December 2018

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

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

Download

There are no files associated with this item.


Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.

Updated:  27 November 2018/ Responsible Officer:  University Librarian/ Page Contact:  Library Systems & Web Coordinator