• DOI:10.1051/0004-6361/201730687
• Corpus ID: 118883548

Luminosities and infrared excess in Type II and anomalous Cepheids in the Large and Small Magellanic Clouds

@article{Groenewegen2017LuminositiesAI,
  title={Luminosities and infrared excess in Type II and anomalous Cepheids in the Large and Small Magellanic Clouds},
  author={Martin A. T. Groenewegen and M. I. Jurkovic},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2017}
}

• M. Groenewegen, M. Jurkovic
• Published 2 May 2017
• Physics
• arXiv: Solar and Stellar Astrophysics

(abridged) Type II and anomalous Cepheids (ACs) are useful distance indicators when there are too few classical Cepheids or when RR Lyrae stars are too faint. We study the sample of 335 Type II and ACs in the Small and Large MCls detected in OGLE-III data.The SEDs are constructed and fitted with a dust radiative transfer model, thereby leading to a determination of luminosity and effective this http URL addition, a subsample of targets is investigated for possible binarity by looking for the light-time travel effect (LITE). Hertzsprung-Russell diagrams (HRD) are constructed and compared to evolutionary tracks and theoretical instability strips (ISs). In agreement with previous suggestions, the BL Her subclass can be explained by the evolution of $\sim$0.5-0.6~\msol\ stars evolving off the ZAHB and the ACs can be explained by the evolution of $\sim$1.1-2.3~\msol\ stars. The evolution of the W Vir subclass is not clear. A relation to binarity might be at the origin of the W Vir stars, which has already been explicitly suggested for the peculiar W Vir stars. For $\sim60\%$ of the RV Tau and $\sim 10\%$ of the W Vir objects an infrared excess is detected from the SED fitting. A recent result is confirmed that stars exist with luminosities below that predicted from single-star evolution, which show a clear infrared excess, and the shape of the excess suggests a connection to binary evolution. The investigation of the LITE effect revealed 20 systems that appear to show periodic variations and may be new binaries, although this study requires follow-up. About 40 stars show significant period changes.