The detailed forms of the LMC Cepheid PL and PLC relations

C. Koen, S. Kanbur, C. Ngeow

Research output: Contribution to journalArticlepeer-review

18 Scopus citations

Abstract

Possible deviations from linearity of the Large Magellanic Cloud Cepheid period-luminosity (PL) and period-luminosity-colour (PLC) relations are investigated. Two data sets are studied, respectively from the Optical Gravitational Lensing Experiment (OGLE) and MACHO projects. A non-parametric test, based on linear regression residuals, suggests that neither PL relation is linear. If colour dependence is allowed for, then the MACHO PL relation is found to deviate more significantly from the linear, while the OGLE PL relation is consistent with linearity. These findings are confirmed by fitting 'Generalized Additive Models' (non-parametric regression functions) to the two data sets. Colour dependence is shown to be non-linear in both data sets, distinctly so in the case of the MACHO Cepheids. It is also shown that there is interaction between the period and the colour functions in the MACHO data.

Original languageEnglish
Pages (from-to)1440-1448
Number of pages9
JournalMonthly Notices of the Royal Astronomical Society
Volume380
Issue number4
DOIs
StatePublished - Oct 2007

Keywords

  • Cepheids
  • Distance scale
  • Methods: statistical

Fingerprint

Dive into the research topics of 'The detailed forms of the LMC Cepheid PL and PLC relations'. Together they form a unique fingerprint.

Cite this