<?xml version="1.0" encoding="utf-8"?>
<TEI xmlns="http://www.tei-c.org/ns/1.0" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:hal="http://hal.archives-ouvertes.fr/" xmlns:gml="http://www.opengis.net/gml/3.3/" xmlns:gmlce="http://www.opengis.net/gml/3.3/ce" version="1.1" xsi:schemaLocation="http://www.tei-c.org/ns/1.0 http://api.archives-ouvertes.fr/documents/aofr-sword.xsd">
  <teiHeader>
    <fileDesc>
      <titleStmt>
        <title>HAL TEI export of hal-04111348</title>
      </titleStmt>
      <publicationStmt>
        <distributor>CCSD</distributor>
        <availability status="restricted">
          <licence target="https://creativecommons.org/publicdomain/zero/1.0/">CC0 1.0 - Universal</licence>
        </availability>
        <date when="2026-05-25T09:35:36+02:00"/>
      </publicationStmt>
      <sourceDesc>
        <p part="N">HAL API Platform</p>
      </sourceDesc>
    </fileDesc>
  </teiHeader>
  <text>
    <body>
      <listBibl>
        <biblFull>
          <titleStmt>
            <title xml:lang="en">Atmospheric escape from hot Jupiters</title>
            <author role="aut">
              <persName>
                <forename type="first">A.</forename>
                <surname>Lecavelier des Etangs</surname>
              </persName>
              <idno type="idhal" notation="numeric">756677</idno>
              <idno type="halauthorid" notation="string">2717671-756677</idno>
              <idno type="ORCID">https://orcid.org/0000-0002-5637-5253</idno>
              <idno type="VIAF">https://viaf.org/viaf/71680464</idno>
              <idno type="IDREF">https://www.idref.fr/083727299</idno>
              <affiliation ref="#struct-541701"/>
            </author>
            <author role="aut">
              <persName>
                <forename type="first">A.</forename>
                <surname>Vidal-Madjar</surname>
              </persName>
              <idno type="halauthorid">72192-0</idno>
              <affiliation ref="#struct-541701"/>
            </author>
            <author role="aut">
              <persName>
                <forename type="first">J. C.</forename>
                <surname>Mcconnell</surname>
              </persName>
              <idno type="halauthorid">141991-0</idno>
            </author>
            <author role="aut">
              <persName>
                <forename type="first">G.</forename>
                <surname>Hébrard</surname>
              </persName>
              <idno type="halauthorid">109625-0</idno>
              <affiliation ref="#struct-541701"/>
            </author>
            <editor role="depositor">
              <persName>
                <forename>Gestionnaire HAL 5</forename>
                <surname>Sorbonne Université</surname>
              </persName>
              <email type="md5">7cfd4753d4999726e403d99c5b54331a</email>
              <email type="domain">sorbonne-universite.fr</email>
            </editor>
          </titleStmt>
          <editionStmt>
            <edition n="v1" type="current">
              <date type="whenSubmitted">2023-06-07 16:06:55</date>
              <date type="whenModified">2025-08-19 10:12:15</date>
              <date type="whenReleased">2023-06-07 16:06:56</date>
              <date type="whenProduced">2004</date>
              <date type="whenEndEmbargoed">2023-06-07</date>
              <ref type="file" target="https://hal.science/hal-04111348v1/document">
                <date notBefore="2023-06-07"/>
              </ref>
              <ref type="file" subtype="greenPublisher" n="1" target="https://hal.science/hal-04111348v1/file/aafk101.pdf" id="file-4121192-3587511">
                <date notBefore="2023-06-07"/>
              </ref>
              <ref type="externalLink" target="http://arxiv.org/pdf/astro-ph/0403369"/>
            </edition>
            <respStmt>
              <resp>contributor</resp>
              <name key="688443">
                <persName>
                  <forename>Gestionnaire HAL 5</forename>
                  <surname>Sorbonne Université</surname>
                </persName>
                <email type="md5">7cfd4753d4999726e403d99c5b54331a</email>
                <email type="domain">sorbonne-universite.fr</email>
              </name>
            </respStmt>
          </editionStmt>
          <publicationStmt>
            <distributor>CCSD</distributor>
            <idno type="halId">hal-04111348</idno>
            <idno type="halUri">https://hal.science/hal-04111348</idno>
            <idno type="halBibtex">lecavelierdesetangs:hal-04111348</idno>
            <idno type="halRefHtml">&lt;i&gt;Astronomy &amp; Astrophysics - A&amp;A&lt;/i&gt;, 2004, 418, pp.L1-L4. &lt;a target="_blank" href="https://dx.doi.org/10.1051/0004-6361:20040106"&gt;&amp;#x27E8;10.1051/0004-6361:20040106&amp;#x27E9;&lt;/a&gt;</idno>
            <idno type="halRef">Astronomy &amp; Astrophysics - A&amp;A, 2004, 418, pp.L1-L4. &amp;#x27E8;10.1051/0004-6361:20040106&amp;#x27E9;</idno>
            <availability status="restricted">
              <licence target="https://about.hal.science/hal-authorisation-v1/">HAL Authorization<ref corresp="#file-4121192-3587511"/></licence>
            </availability>
          </publicationStmt>
          <seriesStmt>
            <idno type="stamp" n="INSU">INSU - Institut National des Sciences de l'Univers</idno>
            <idno type="stamp" n="CNRS">CNRS - Centre national de la recherche scientifique</idno>
            <idno type="stamp" n="IAP" corresp="SORBONNE-UNIVERSITE">Institut d'Astrophysique de Paris</idno>
            <idno type="stamp" n="SORBONNE-UNIVERSITE">Sorbonne Université</idno>
            <idno type="stamp" n="SU-INF-2018" corresp="SORBONNE-UNIVERSITE">SORBONNE université &lt;2018</idno>
            <idno type="stamp" n="SU-SCIENCES" corresp="SORBONNE-UNIVERSITE">Faculté des Sciences de Sorbonne Université</idno>
            <idno type="stamp" n="SU-TI">Sorbonne Université - Texte Intégral</idno>
            <idno type="stamp" n="ALLIANCE-SU"> Alliance Sorbonne Université</idno>
          </seriesStmt>
          <notesStmt>
            <note type="audience" n="2">International</note>
            <note type="popular" n="0">No</note>
            <note type="peer" n="1">Yes</note>
          </notesStmt>
          <sourceDesc>
            <biblStruct>
              <analytic>
                <title xml:lang="en">Atmospheric escape from hot Jupiters</title>
                <author role="aut">
                  <persName>
                    <forename type="first">A.</forename>
                    <surname>Lecavelier des Etangs</surname>
                  </persName>
                  <idno type="idhal" notation="numeric">756677</idno>
                  <idno type="halauthorid" notation="string">2717671-756677</idno>
                  <idno type="ORCID">https://orcid.org/0000-0002-5637-5253</idno>
                  <idno type="VIAF">https://viaf.org/viaf/71680464</idno>
                  <idno type="IDREF">https://www.idref.fr/083727299</idno>
                  <affiliation ref="#struct-541701"/>
                </author>
                <author role="aut">
                  <persName>
                    <forename type="first">A.</forename>
                    <surname>Vidal-Madjar</surname>
                  </persName>
                  <idno type="halauthorid">72192-0</idno>
                  <affiliation ref="#struct-541701"/>
                </author>
                <author role="aut">
                  <persName>
                    <forename type="first">J. C.</forename>
                    <surname>Mcconnell</surname>
                  </persName>
                  <idno type="halauthorid">141991-0</idno>
                </author>
                <author role="aut">
                  <persName>
                    <forename type="first">G.</forename>
                    <surname>Hébrard</surname>
                  </persName>
                  <idno type="halauthorid">109625-0</idno>
                  <affiliation ref="#struct-541701"/>
                </author>
              </analytic>
              <monogr>
                <idno type="halJournalId" status="VALID">10858</idno>
                <idno type="issn">0004-6361</idno>
                <idno type="eissn">1432-0746</idno>
                <title level="j">Astronomy &amp; Astrophysics - A&amp;A</title>
                <imprint>
                  <publisher>EDP Sciences</publisher>
                  <biblScope unit="volume">418</biblScope>
                  <biblScope unit="pp">L1-L4</biblScope>
                  <date type="datePub">2004</date>
                </imprint>
              </monogr>
              <idno type="arxiv">astro-ph/0403369</idno>
              <idno type="bibcode">2004A&amp;A...418L...1L</idno>
              <idno type="doi">10.1051/0004-6361:20040106</idno>
            </biblStruct>
          </sourceDesc>
          <profileDesc>
            <langUsage>
              <language ident="en">English</language>
            </langUsage>
            <textClass>
              <keywords scheme="author">
                <term xml:lang="en">star: individual: HD 209458</term>
                <term xml:lang="en">stars: planetary systems</term>
                <term xml:lang="en">Astrophysics</term>
              </keywords>
              <classCode scheme="halDomain" n="sdu">Sciences of the Universe [physics]</classCode>
              <classCode scheme="halTypology" n="ART">Journal articles</classCode>
              <classCode scheme="halOldTypology" n="ART">Journal articles</classCode>
              <classCode scheme="halTreeTypology" n="ART">Journal articles</classCode>
            </textClass>
            <abstract xml:lang="en">
              <p>The extra-solar planet HD 209458b has been found to have an extended atmosphere of escaping atomic hydrogen (Vidal-Madjar et al. 2003), suggesting that ``hot Jupiters'' closer to their parent stars could evaporate. Here we estimate the atmospheric escape (so called evaporation rate) from hot Jupiters and their corresponding life time against evaporation. The calculated evaporation rate of HD 209458b is in excellent agreement with the H I Lyman-α observations. We find that the tidal forces and high temperatures in the upper atmosphere must be taken into account to obtain reliable estimate of the atmospheric escape. Because of the tidal forces, we show that there is a new escape mechanism at intermediate temperatures at which the exobase reaches the Roche lobe. From an energy balance, we can estimate plausible values for the planetary exospheric temperatures, and thus obtain typical life times of planets as a function of their mass and orbital distance.</p>
            </abstract>
          </profileDesc>
        </biblFull>
      </listBibl>
    </body>
    <back>
      <listOrg type="structures">
        <org type="laboratory" xml:id="struct-541701" status="VALID">
          <idno type="IdRef">028182030</idno>
          <idno type="ISNI">0000000105408249</idno>
          <idno type="RNSR">200112483U</idno>
          <idno type="ROR">022bnxw24</idno>
          <orgName>Institut d'Astrophysique de Paris</orgName>
          <orgName type="acronym">IAP</orgName>
          <date type="start">2018-01-01</date>
          <desc>
            <address>
              <addrLine>98bis, bd Arago - 75014 Paris France</addrLine>
              <country key="FR"/>
            </address>
            <ref type="url">http://www.iap.fr/</ref>
          </desc>
          <listRelation>
            <relation name="UMR7095" active="#struct-300045" type="direct"/>
            <relation active="#struct-413221" type="direct"/>
            <relation name="UMR7095" active="#struct-441569" type="direct"/>
          </listRelation>
        </org>
        <org type="institution" xml:id="struct-300045" status="VALID">
          <idno type="IdRef">029349265</idno>
          <idno type="ISNI">0000 0001 2154 1736</idno>
          <idno type="ROR">https://ror.org/04kdfz702</idno>
          <idno type="Wikidata">Q3152437</idno>
          <orgName>Institut national des sciences de l'Univers</orgName>
          <orgName type="acronym">INSU - CNRS</orgName>
          <date type="start">2007-04-19</date>
          <desc>
            <address>
              <addrLine>INSU-CNRS3 rue Michel-Ange, 75794 Paris Cedex 16</addrLine>
              <country key="FR"/>
            </address>
            <ref type="url">https://www.insu.cnrs.fr</ref>
          </desc>
        </org>
        <org type="regroupinstitution" xml:id="struct-413221" status="VALID">
          <idno type="IdRef">221333754</idno>
          <idno type="ROR">https://ror.org/02en5vm52</idno>
          <orgName>Sorbonne Université</orgName>
          <orgName type="acronym">SU</orgName>
          <date type="start">2018-01-01</date>
          <desc>
            <address>
              <addrLine>21 rue de l’École de médecine - 75006 Paris</addrLine>
              <country key="FR"/>
            </address>
            <ref type="url">http://www.sorbonne-universite.fr/</ref>
          </desc>
        </org>
        <org type="regroupinstitution" xml:id="struct-441569" status="VALID">
          <idno type="IdRef">02636817X</idno>
          <idno type="ISNI">0000000122597504</idno>
          <idno type="ROR">https://ror.org/02feahw73</idno>
          <orgName>Centre National de la Recherche Scientifique</orgName>
          <orgName type="acronym">CNRS</orgName>
          <date type="start">1939-10-19</date>
          <desc>
            <address>
              <country key="FR"/>
            </address>
            <ref type="url">https://www.cnrs.fr/</ref>
          </desc>
        </org>
      </listOrg>
    </back>
  </text>
</TEI>