Ontology type: schema:ScholarlyArticle
2021-06
AUTHORS ABSTRACTThe reduction of all the available photometry for the Cepheid CE Pup has allowed its \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$O-C$$\end{document} diagram spanning a time interval of 128 years to be constructed. This has made it possible for the first time to calculate the rate of evolutionary increase in the period, \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$dP/dt=+155.3(\pm{13.1})$$\end{document} s yr\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${}^{-1}$$\end{document}, in agreement the results of model calculations for the third crossing of the instability strip. The pulsation stability test proposed by Lombard and Koen confirmed that the evolutionary change in the period is real. More... »
PAGES420-429
http://scigraph.springernature.com/pub.10.1134/s1063773721060025
DOIhttp://dx.doi.org/10.1134/s1063773721060025
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