Period–colour and amplitude–colour relations in classical Cepheid variables – V. The Small Magellanic Cloud Cepheid models
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/380/2/819/18428443/mnras0380-0819.pdf
Reference34 articles.
1. Cepheid mass-luminosity relations from the Magellanic Clouds
2. Intermediate‐Mass Star Models with Different Helium and Metal Contents
3. Cepheids in the Magellanic Clouds
4. A Note on the Period-Spectrum Relation among Cepheids.
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2. Geometry of the LMC based on multiphase analysis of multiwavelength Cepheid light curves using OGLE-IV and Gaia DR3 data;Monthly Notices of the Royal Astronomical Society;2023-11-27
3. A multiphase study of theoretical and observed light curves of classical Cepheids in the Magellanic Clouds;Monthly Notices of the Royal Astronomical Society;2023-03-17
4. The stellar photosphere–hydrogen ionization front interaction in classical pulsators: a theoretical explanation for observed period–colour relations;Monthly Notices of the Royal Astronomical Society;2020-01-22
5. PERIOD–COLOR AND AMPLITUDE–COLOR RELATIONS AT MAXIMUM AND MINIMUM LIGHT FOR RR LYRAE STARS IN THE SDSS STRIPE 82 REGION;The Astrophysical Journal;2017-01-10
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