<?xml version="1.0" encoding="UTF-8"?>

<modsCollection xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.loc.gov/mods/v3" xsi:schemaLocation="http://www.loc.gov/mods/v3 http://www.loc.gov/standards/mods/v3/mods-3-3.xsd">
<mods version="3.3">

<genre>article</genre>

<titleInfo><title>Probing the internal magnetism of stars using asymptotic magneto-asteroseismology</title></titleInfo>


<note type="publicationStatus">published</note>


<note type="qualityControlled">yes</note>

<name type="personal">
  <namePart type="given">S.</namePart>
  <namePart type="family">Mathis</namePart>
  <role><roleTerm type="text">author</roleTerm> </role></name>
<name type="personal">
  <namePart type="given">Lisa Annabelle</namePart>
  <namePart type="family">Bugnet</namePart>
  <role><roleTerm type="text">author</roleTerm> </role><identifier type="local">d9edb345-f866-11ec-9b37-d119b5234501</identifier><description xsi:type="identifierDefinition" type="orcid">0000-0003-0142-4000</description></name>
<name type="personal">
  <namePart type="given">V.</namePart>
  <namePart type="family">Prat</namePart>
  <role><roleTerm type="text">author</roleTerm> </role></name>
<name type="personal">
  <namePart type="given">K.</namePart>
  <namePart type="family">Augustson</namePart>
  <role><roleTerm type="text">author</roleTerm> </role></name>
<name type="personal">
  <namePart type="given">S.</namePart>
  <namePart type="family">Mathur</namePart>
  <role><roleTerm type="text">author</roleTerm> </role></name>
<name type="personal">
  <namePart type="given">R. A.</namePart>
  <namePart type="family">Garcia</namePart>
  <role><roleTerm type="text">author</roleTerm> </role></name>














<abstract lang="eng">Context. Our knowledge of the dynamics of stars has undergone a revolution through the simultaneous large amount of high-quality photometric observations collected by space-based asteroseismology and ground-based high-precision spectropolarimetry. They allowed us to probe the internal rotation of stars and their surface magnetism in the whole Hertzsprung-Russell diagram. However, new methods should still be developed to probe the deep magnetic fields in these stars.

Aims. Our goal is to provide seismic diagnoses that allow us to probe the internal magnetism of stars.

Methods. We focused on asymptotic low-frequency gravity modes and high-frequency acoustic modes. Using a first-order perturbative theory, we derived magnetic splittings of their frequencies as explicit functions of stellar parameters.

Results. As in the case of rotation, we show that asymptotic gravity and acoustic modes can allow us to probe the different components of the magnetic field in the cavities in which they propagate. This again demonstrates the high potential of using mixed-modes when this is possible.</abstract>

<originInfo><publisher>EDP Sciences</publisher><dateIssued encoding="w3cdtf">2021</dateIssued>
</originInfo>
<language><languageTerm authority="iso639-2b" type="code">eng</languageTerm>
</language>

<subject><topic>Space and Planetary Science</topic><topic>Astronomy and Astrophysics</topic><topic>asteroseismology / waves / stars</topic><topic>magnetic field / stars</topic><topic>oscillations / methods</topic><topic>analytical</topic>
</subject>


<relatedItem type="host"><titleInfo><title>Astronomy &amp; Astrophysics</title></titleInfo>
  <identifier type="issn">0004-6361</identifier>
  <identifier type="eIssn">1432-0746</identifier>
  <identifier type="arXiv">2012.11050</identifier><identifier type="doi">10.1051/0004-6361/202039180</identifier>
<part><detail type="volume"><number>647</number></detail>
</part>
</relatedItem>

<note type="extern">yes</note>
<extension>
<bibliographicCitation>
<ista>Mathis S, Bugnet LA, Prat V, Augustson K, Mathur S, Garcia RA. 2021. Probing the internal magnetism of stars using asymptotic magneto-asteroseismology. Astronomy &amp;#38; Astrophysics. 647, A122.</ista>
<mla>Mathis, S., et al. “Probing the Internal Magnetism of Stars Using Asymptotic Magneto-Asteroseismology.” &lt;i&gt;Astronomy &amp;#38; Astrophysics&lt;/i&gt;, vol. 647, A122, EDP Sciences, 2021, doi:&lt;a href=&quot;https://doi.org/10.1051/0004-6361/202039180&quot;&gt;10.1051/0004-6361/202039180&lt;/a&gt;.</mla>
<ama>Mathis S, Bugnet LA, Prat V, Augustson K, Mathur S, Garcia RA. Probing the internal magnetism of stars using asymptotic magneto-asteroseismology. &lt;i&gt;Astronomy &amp;#38; Astrophysics&lt;/i&gt;. 2021;647. doi:&lt;a href=&quot;https://doi.org/10.1051/0004-6361/202039180&quot;&gt;10.1051/0004-6361/202039180&lt;/a&gt;</ama>
<short>S. Mathis, L.A. Bugnet, V. Prat, K. Augustson, S. Mathur, R.A. Garcia, Astronomy &amp;#38; Astrophysics 647 (2021).</short>
<chicago>Mathis, S., Lisa Annabelle Bugnet, V. Prat, K. Augustson, S. Mathur, and R. A. Garcia. “Probing the Internal Magnetism of Stars Using Asymptotic Magneto-Asteroseismology.” &lt;i&gt;Astronomy &amp;#38; Astrophysics&lt;/i&gt;. EDP Sciences, 2021. &lt;a href=&quot;https://doi.org/10.1051/0004-6361/202039180&quot;&gt;https://doi.org/10.1051/0004-6361/202039180&lt;/a&gt;.</chicago>
<ieee>S. Mathis, L. A. Bugnet, V. Prat, K. Augustson, S. Mathur, and R. A. Garcia, “Probing the internal magnetism of stars using asymptotic magneto-asteroseismology,” &lt;i&gt;Astronomy &amp;#38; Astrophysics&lt;/i&gt;, vol. 647. EDP Sciences, 2021.</ieee>
<apa>Mathis, S., Bugnet, L. A., Prat, V., Augustson, K., Mathur, S., &amp;#38; Garcia, R. A. (2021). Probing the internal magnetism of stars using asymptotic magneto-asteroseismology. &lt;i&gt;Astronomy &amp;#38; Astrophysics&lt;/i&gt;. EDP Sciences. &lt;a href=&quot;https://doi.org/10.1051/0004-6361/202039180&quot;&gt;https://doi.org/10.1051/0004-6361/202039180&lt;/a&gt;</apa>
</bibliographicCitation>
</extension>
<recordInfo><recordIdentifier>11606</recordIdentifier><recordCreationDate encoding="w3cdtf">2022-07-18T12:15:27Z</recordCreationDate><recordChangeDate encoding="w3cdtf">2024-10-14T11:39:21Z</recordChangeDate>
</recordInfo>
</mods>
</modsCollection>
