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Eclipsing Binaries with Classical Cepheid Component in the Magellanic System

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arxiv 1601.01683 v1 pith:AP4FXZBT submitted 2016-01-07 astro-ph.SR

Eclipsing Binaries with Classical Cepheid Component in the Magellanic System

classification astro-ph.SR
keywords cepheidseclipsingclassicalsystemsystemsbinarycepheidcomponent
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We present a census of eclipsing binary systems with classical Cepheid as a component. All such systems known were found in the OGLE collection of classical Cepheids in the Magellanic System. We extend the list of potential candidates adding four new objects found in the OGLE-IV photometric data. One of the new Cepheids in the eclipsing system, OGLE-SMC-CEP-3235, revealed only one eclipse during 15 years of the OGLE photometric monitoring. However, it additionally shows very well pronounced light-time effect indicating that the binarity is real. We also search for the light-time effect in other known eclipsing Cepheids and we clearly detect it in OGLE-LMC-CEP-1812. We discuss application of this tool for the search for Cepheids in non-eclipsing binary systems.

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  1. Connecting Stellar Population Surveys to Stellar Evolution with Delay-time Distributions: Application to LMC Classical Cepheids

    astro-ph.SR 2026-06 unverdicted novelty 5.0

    DTDs measured for LMC Cepheids recover progenitor age ranges consistent with non-canonical period-age relations that include overshooting and rotation.