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A tidally tilted sectoral dipole pulsation mode in the eclipsing binary TIC 63328020

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F21%3A00548962" target="_blank" >RIV/67985815:_____/21:00548962 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216224:14310/21:00121712

  • Result on the web

    <a href="https://doi.org/10.1093/mnras/stab336" target="_blank" >https://doi.org/10.1093/mnras/stab336</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1093/mnras/stab336" target="_blank" >10.1093/mnras/stab336</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    A tidally tilted sectoral dipole pulsation mode in the eclipsing binary TIC 63328020

  • Original language description

    We report the discovery of the third tidally tilted pulsator, TIC 63328020. Observations with the TESS satellite reveal binary eclipses with an orbital period of 1.1057 d, and delta Scuti-type pulsations with a mode frequency of 21.09533 d(-1). This pulsation exhibits a septuplet of orbital sidelobes as well as a harmonic quintuplet. Using the oblique pulsatormodel, the primary oscillation is identified as a sectoral dipole mode with l = 1, vertical bar m vertical bar = 1. We find the pulsating star to have M-1 similar or equal to 2.5M(circle dot), R-1 similar or equal to 3R(circle dot), and T-eff, 1 similar or equal to 8000 K, while the secondary has M-2 similar or equal to 1.1M(circle dot), R-2 similar or equal to 2R(circle dot), and T-eff, 2 similar or equal to 5600 K. Both stars appear to be close to filling their respective Roche lobes. The properties of this binary as well as the tidally tilted pulsations differ from the previous two tidally tilted pulsators, HD74423 and CO Cam, in important ways. We also study the prior history of this system with binary evolution models and conclude that extensive mass transfer has occurred from the current secondary to the primary.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/EF16_027%2F0008360" target="_blank" >EF16_027/0008360: Postdoc@MUNI</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2021

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Monthly Notices of the Royal Astronomical Society

  • ISSN

    0035-8711

  • e-ISSN

    1365-2966

  • Volume of the periodical

    503

  • Issue of the periodical within the volume

    1

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    16

  • Pages from-to

    254-69

  • UT code for WoS article

    000641987400016

  • EID of the result in the Scopus database

    2-s2.0-85105214384