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Discovery of pulsating components in eclipsing binary systems through the TESS light curves: the cases of CPD-30 740, HD 97329, V1637 Ori and TYC 683-640-1

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Abstract

We present the first evidence for the pulsations of primary components of four eclipsing binary systems. The TESS light curves of the targets are analyzed, the light and the absolute parameters are derived. Fourier analyses are applied to the residual data subtracted from the binary models to reveal the pulsational characteristics of the primaries. The components of the systems are compared to well-known binary systems of the same morphological type. The types of pulsational classes for the primaries are also discussed. Results show that CPD-30 740 and V1637 Ori are oscillating eclipsing Algol type binary stars, while HD 97329 and TYC 683-640-1 are found to be detached systems with pulsating primary components. We conclude that the primary components of the systems are pulsating stars.

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Notes

  1. mast.stsci.edu/portal/Mashup/Clients/Mast/Portal.html.

  2. https://irsa.ipac.caltech.edu/applications/DUST/.

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Acknowledgements

The authors would like to thank Dr. David Mkrtichian for his valuable comments and suggestions. CU acknowledges the research grant No. R00125 administered by the office of the DVC Research, Development and Innovation at Botswana International University of Science and Technology (BIUST). Southern Cross Astronomy Research Group would like to thank BIUST for the support from grant No. R00125. This paper includes data collected with the TESS mission, obtained from the MAST data archive at the Space Telescope Science Institute (STScI). Funding for the TESS mission is provided by the NASA Explorer Program. STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France. Some/all of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non-HST data is provided by the NASA Office of Space Science via grant NNX13AC07G and by other grants and contracts. This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France. This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. This work has made use of the NASA/IPAC Infrared Science Archive, which is funded by the National Aeronautics and Space Administration and operated by the California Institute of Technology.

Funding

This work was funded by Botswana International University of Science and Technology (BIUST) (Grant number R00125).

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  1. Department of Space Sciences and Technologies, Faculty of Arts and Sciences, Çanakkale Onsekiz Mart University, Terzioǧlu Campus, 17100, Çanakkale, Turkey

    Burak Ulaş

  2. Astrophysics Research Centre and Observatory, Çanakkale Onsekiz Mart University, Terzioǧlu Campus, 17100, Çanakkale, Turkey

    Burak Ulaş & Naci Erkan

  3. Department of Physics and Astronomy, Botswana International University of Science and Technology (BIUST), Plot 10017, Private Bag 16, Palapye, Botswana

    Ceren Ulusoy, Mothusi Madiba & Mercy Matsete

  4. Department of Physics, Faculty of Arts and Sciences, Çanakkale Onsekiz Mart University, Terzioǧlu Campus, 17100, Çanakkale, Turkey

    Naci Erkan

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Appendix: List of combined frequencies

Appendix: List of combined frequencies

Table 5 shows the possible combination frequencies of the primary components of the systems as a continuation of Table 3. The combination relations are denoted in the first column.

Table 5 Combination frequencies derived from the frequency analysis of the systems. The standard errors are given in parentheses for the last digits
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Ulaş, B., Ulusoy, C., Erkan, N. et al. Discovery of pulsating components in eclipsing binary systems through the TESS light curves: the cases of CPD-30 740, HD 97329, V1637 Ori and TYC 683-640-1. Astrophys Space Sci 367, 22 (2022). https://doi.org/10.1007/s10509-022-04053-6

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