Distance determination from the Cepheid and RR Lyrae period-luminosity relations

Chow Choong Ngeow, Wolfgang Gieren, Christopher Klein

研究成果: 書貢獻/報告類型會議論文篇章同行評審

1 引文 斯高帕斯(Scopus)

摘要

Cepheids and RR Lyrae stars are important pulsating variable stars in distance scale work because they serve as standard candles. Cepheids follow well-defined period-luminosity (PL) relations defined for bands extending from optical to mid-infrared (MIR). On the other hand, RR Lyrae stars also exhibit PL relations in the near-infrared and MIR wavelengths. In this article, we review some of the recent developments and calibrations of PL relations for Cepheids and RR Lyrae stars. For Cepheids, we discuss the calibration of PL relations via the Galactic and the Large Magellanic Cloud routes. For RR Lyrae stars, we summarize some recent work in developing the MIR PL relations.

原文???core.languages.en_GB???
主出版物標題Precision Asteroseismology
編輯Joyce Guzik, William Chaplin, William Chaplin, Gerald Handler, Andrzej Pigulski
頁面123-128
頁數6
版本S301
DOIs
出版狀態已出版 - 2014

出版系列

名字Proceedings of the International Astronomical Union
號碼S301
9
ISSN(列印)1743-9213
ISSN(電子)1743-9221

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