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Mode identification and period fitting in six pulsating hot subdwarfs

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F24%3A00598898" target="_blank" >RIV/67985815:_____/24:00598898 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1017/pasa.2024.38" target="_blank" >https://doi.org/10.1017/pasa.2024.38</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1017/pasa.2024.38" target="_blank" >10.1017/pasa.2024.38</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Mode identification and period fitting in six pulsating hot subdwarfs

  • Original language description

    We report the results of our analysis of six gravity-mode pulsating hot subdwarf stars observed in the short cadence mode by Transiting Exoplanet Survey Satellite. We detected at least 10 pulsation periods in each star, searched for multiplets, and used an asymptotic period spacing to identify modes. We used a grid of evolutionary and pulsation models calculated with the MESA and GYRE, along with spectroscopic parameters and modal degree identification, to derive the physical properties of the stars. We checked the relation between the helium content and pulsations and found that no pulsator exists among the extremely helium-rich hot subdwarfs, while the number of detected pulsators in other helium groups increases as the helium content decreases. We found p- and g-mode hot subdwarfs pulsators in all Galactic populations.

  • 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/GA22-34467S" target="_blank" >GA22-34467S: Binary interaction on the red giant branch: Hot subdwarfs as a test case.</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2024

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Publications of the Astronomical Society of Australia

  • ISSN

    1323-3580

  • e-ISSN

    1448-6083

  • Volume of the periodical

    41

  • Issue of the periodical within the volume

    May

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    19

  • Pages from-to

    e041

  • UT code for WoS article

    001299164000001

  • EID of the result in the Scopus database

    2-s2.0-85193803359