A new method for determining physical parameters of fundamental mode RR Lyrae stars from multicolour light curves
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/394/1/261/3866798/mnras0394-0261.pdf
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1. The effective temperature scale of giant stars (F0–K5)
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1. Blazhko-type fundamental-mode RR Lyrae stars in the globular cluster M3;Monthly Notices of the Royal Astronomical Society;2019-10-03
2. A cautionary tale of interpreting O−C diagrams: period instability in a classical RR Lyr Star Z CVn mimicking as a distant companion;Monthly Notices of the Royal Astronomical Society;2017-10-24
3. Antarctica photometry of the Blazhko RR Lyrae star S Arae;Monthly Notices of the Royal Astronomical Society;2015-12-14
4. OVERTONE AND MULTI-MODE RR LYRAE STARS IN THE GLOBULAR CLUSTER M3;The Astrophysical Journal Supplement Series;2015-08-11
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