Presentation Open Access

The temperature, gravity, and frequency scaling relation for delta Scuti stars

S. Barceló Forteza; A. Moya; D. Barrado; E. Solano; S. Martín-Ruiz; J.C. Suárez; A. García Hernández


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  <identifier identifierType="DOI">10.5281/zenodo.5560876</identifier>
  <creators>
    <creator>
      <creatorName>S. Barceló Forteza</creatorName>
      <affiliation>Universidad de Granada (UGR)</affiliation>
    </creator>
    <creator>
      <creatorName>A. Moya</creatorName>
    </creator>
    <creator>
      <creatorName>D. Barrado</creatorName>
    </creator>
    <creator>
      <creatorName>E. Solano</creatorName>
    </creator>
    <creator>
      <creatorName>S. Martín-Ruiz</creatorName>
    </creator>
    <creator>
      <creatorName>J.C. Suárez</creatorName>
    </creator>
    <creator>
      <creatorName>A. García Hernández</creatorName>
    </creator>
  </creators>
  <titles>
    <title>The temperature, gravity, and frequency scaling relation for delta Scuti stars</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2021</publicationYear>
  <dates>
    <date dateType="Issued">2021-10-11</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Presentation</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/5560876</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.5560875</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://zenodo.org/communities/plato2021</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="https://creativecommons.org/licenses/by/4.0/legalcode">Creative Commons Attribution 4.0 International</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">&lt;p&gt;Thanks to long-duration high-cadence light curves from space telescopes, we suggest the frequency at maximum power as a proper indicative of the mean temperature and surface gravity for delta Scuti stars. This seismic index do not depend on rotation or inclination unlike photometric and spectroscopic techniques that may be significantly affected by gravity-darkening effect or extinction. Thus, it is posible to improve their distance, age, and habitable zone measurements for this kind of stars.&lt;/p&gt;</description>
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