Pulsation-decline relationships in R Coronae Borealis stars
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/375/1/301/3094866/mnras0375-0301.pdf
Reference21 articles.
1. Dynamical modeling of long-period variable star atmospheres
2. An ultraviolet and visible spectroscopic study of a pulsational cycle of RY Sagittarii
3. The chemical composition of R Coronae Borealis and XX Camelopardalis
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1. ROAD† and K2 photometry of V348 Sgr: probing the pulsation dust connection;Monthly Notices of the Royal Astronomical Society;2019-06-10
2. R Coronae Borealis: radial velocity and other observations, 1950–2007;Monthly Notices of the Royal Astronomical Society;2018-10-30
3. Low-metallicity CO + He WD post-merger models for RCB stars as a source of pre-solar graphite grains;Monthly Notices of the Royal Astronomical Society;2018-09-24
4. The curious case of II Lup: a complex morphology revealed with SAM/NACO and ALMA;Monthly Notices of the Royal Astronomical Society;2018-07-19
5. References;Pulsating Stars;2015-08-21
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