Period-colour and amplitude-colour relations in classical Cepheid variables - VI. New challenges for pulsation models

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题名:	Period-colour and amplitude-colour relations in classical Cepheid variables - VI. New challenges for pulsation models
作者:	Kanbur,SM;Marconi,M;Ngeow,C;Musella,I;Turner,M;James,A;Magin,S;Halsey,J
贡献者:	天文研究所
关键词:	LUMINOSITY RELATIONS;MAGELLANIC CLOUDS;HUBBLE CONSTANT;IA SUPERNOVAE;STARS;METALLICITY;CONVECTION;STABILITY;LMC
日期:	2010
上传时间:	2012-03-27 18:09:46 (UTC+8)
出版者:	國立中央大學
摘要:	We present multiphase period-colour/amplitude-colour/period-luminosity relations using the Optical Gravitational Lensing Experiment III (OGLE III) and Galactic Cepheid data and compare with state of the art theoretical pulsation models. Using this new way to compare models and observations, we find convincing evidence that both period-colour and period-luminosity relations as a function of phase are dynamic and highly non-linear at certain pulsation phases. We extend this to a multiphase Wesenheit function and find the same result. Hence our results cannot be due to reddening errors. We present statistical tests and movies depicting the period-colour/period-luminosity and Wesenheit relations as a function of phase for the Large Magellanic Cloud (LMC) OGLE III Cepheid data: these tests and movies clearly demonstrate non-linearity as a function of phase and offer a new window towards a deeper understanding of stellar pulsation. When comparing with models, we find that the models also predict this non-linearity in both period-colour and period-luminosity planes. The models with (Z = 0.004, Y = 0.25) fare better in mimicking the LMC Cepheid relations, particularly at longer periods, though the models predict systematically higher amplitudes than the observations.
關聯:	MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
显示于类别:	[天文研究所] 期刊論文

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