Period Changes of LMC Cepheids in the OGLE and MACHO Data
Radoslaw Poleski

TL;DR
This study analyzes period changes in LMC Cepheids using OGLE and MACHO data, revealing that overtone pulsators are less stable and that short-term fluctuations dominate long-term period change diagrams.
Contribution
It provides a comparative analysis of period changes in Cepheids from OGLE and MACHO data, highlighting the prevalence of nonlinear and random fluctuations over decades.
Findings
41% of first overtone Cepheids show period changes
No correlation between OGLE and MACHO period change signs
Short-term fluctuations dominate long-term period change diagrams
Abstract
Pulsation period of Cepheids should change as stars evolve through the instability strip. Rates of these changes found by other authors based on the decades-long O-C diagrams show rather good agreement with theoretical predictions. We have checked the variability on the scale of a few years on the data recently published by the Optical Gravitational Lensing Experiment (OGLE) for the Large Magellanic Cloud Cepheids and found period changes for 18% of fundamental mode and 41% of first overtone pulsators. It suggest the overtone pulsations are less stable than the fundamental ones. For stars which had the cross-references in the MACHO catalog we have checked if the period change rates derived from the OGLE and the MACHO data are consistent. It was found that there is no correlation and opposite signs of changes in both data sets are more common than the same ones. Many O-C diagrams show…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Adaptive optics and wavefront sensing
