On the second-overtone stability among Small Magellanic Cloud Cepheids
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/325/4/1353/3033551/325-4-1353.pdf
Reference29 articles.
1. The MACHO Project LMC Variable Star Inventory. VIII. The Recent Star Formation History of the Large Magellanic Cloud from the Cepheid Period Distribution
2. The characteristics of second-overtone-mode Cepheids predicted by non-linear pulsation models
3. The two period-luminosity relations for population I Cepheids
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