<?xml version="1.0" encoding="UTF-8"?>
<record
    xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
    xsi:schemaLocation="http://www.loc.gov/MARC21/slim http://www.loc.gov/standards/marcxml/schema/MARC21slim.xsd"
    xmlns="http://www.loc.gov/MARC21/slim">

  <leader>03069nam a22004455i 4500</leader>
  <controlfield tag="001">978-1-4020-5803-5</controlfield>
  <controlfield tag="003">DE-He213</controlfield>
  <controlfield tag="005">20260521092128.0</controlfield>
  <controlfield tag="007">cr nn 008mamaa</controlfield>
  <controlfield tag="008">100301s2010    ne |    s    |||| 0|eng d</controlfield>
  <datafield tag="020" ind1=" " ind2=" ">
    <subfield code="a">9781402058035</subfield>
  </datafield>
  <datafield tag="020" ind1=" " ind2=" ">
    <subfield code="a">99781402058035</subfield>
  </datafield>
  <datafield tag="024" ind1="7" ind2=" ">
    <subfield code="a">10.1007/978-1-4020-5803-5</subfield>
    <subfield code="2">doi</subfield>
  </datafield>
  <datafield tag="082" ind1="0" ind2="4">
    <subfield code="a">520</subfield>
    <subfield code="2">23</subfield>
  </datafield>
  <datafield tag="100" ind1="1" ind2=" ">
    <subfield code="a">Aerts, C.</subfield>
    <subfield code="e">author.</subfield>
  </datafield>
  <datafield tag="245" ind1="1" ind2="0">
    <subfield code="a">Asteroseismology</subfield>
    <subfield code="h">[electronic resource] /</subfield>
    <subfield code="c">by C. Aerts, J. Christensen-Dalsgaard, D. W. Kurtz.</subfield>
  </datafield>
  <datafield tag="264" ind1=" " ind2="1">
    <subfield code="a">Dordrecht :</subfield>
    <subfield code="b">Springer Netherlands :</subfield>
    <subfield code="b">Imprint: Springer,</subfield>
    <subfield code="c">2010.</subfield>
  </datafield>
  <datafield tag="300" ind1=" " ind2=" ">
    <subfield code="a">XVI, 866p.</subfield>
    <subfield code="b">online resource.</subfield>
  </datafield>
  <datafield tag="336" ind1=" " ind2=" ">
    <subfield code="a">text</subfield>
    <subfield code="b">txt</subfield>
    <subfield code="2">rdacontent</subfield>
  </datafield>
  <datafield tag="337" ind1=" " ind2=" ">
    <subfield code="a">computer</subfield>
    <subfield code="b">c</subfield>
    <subfield code="2">rdamedia</subfield>
  </datafield>
  <datafield tag="338" ind1=" " ind2=" ">
    <subfield code="a">online resource</subfield>
    <subfield code="b">cr</subfield>
    <subfield code="2">rdacarrier</subfield>
  </datafield>
  <datafield tag="347" ind1=" " ind2=" ">
    <subfield code="a">text file</subfield>
    <subfield code="b">PDF</subfield>
    <subfield code="2">rda</subfield>
  </datafield>
  <datafield tag="490" ind1="1" ind2=" ">
    <subfield code="a">Astronomy and Astrophysics Library,</subfield>
    <subfield code="x">0941-7834</subfield>
  </datafield>
  <datafield tag="505" ind1="0" ind2=" ">
    <subfield code="a">Preface -- 1 Introducing asteroseismology -- 2 Stellar oscillations across the Hertzsprung-Russell Diagram -- 3 Theory of stellar oscillations -- 4 Observational techniques -- 5 Frequency analysis -- 6 Modeidentification -- 7 Applications of asteroseismology -- 8 Thefuture -- Bibliography -- A Summary of the different classes of stellar pulsators -- B Properties of Legendre functions and spherical harmonics -- C Mathematical preliminaries -- D Adiabatic oscillations in an isothermal atmosphere -- E Asymptotic theory of stellar oscillations -- Subject index -- Object index -- Acronym definition index.</subfield>
  </datafield>
  <datafield tag="520" ind1=" " ind2=" ">
    <subfield code="a">The recent research domain of asteroseismology studies the internal structure of stars, which is not directly observable, through the interpretation of the frequency spectra of stellar oscillations. The basic principles of asteroseismology are very similar to those developed by earth seismologists. Stellar interiors can be probed from oscillations because different oscillation modes penetrate to different depths inside the star. Asteroseismology is the only available method to derive the internal structure of the stars with high precision. This book - the first on asteroseismology - offers a practical guide for graduate students and scientists working in stellar astrophysics. It provides a general introduction to asteroseismology and comprehensive coverage of all its aspects: fundamental theory, observations and observational techniques, methodology of data analysis and seismic interpretations of various classes of multi-periodic pulsating stars.</subfield>
  </datafield>
  <datafield tag="650" ind1=" " ind2="0">
    <subfield code="a">PHYSICS.</subfield>
  </datafield>
  <datafield tag="650" ind1=" " ind2="0">
    <subfield code="a">ASTRONOMY.</subfield>
  </datafield>
  <datafield tag="650" ind1="1" ind2="4">
    <subfield code="a">PHYSICS.</subfield>
  </datafield>
  <datafield tag="650" ind1="2" ind2="4">
    <subfield code="a">ASTRONOMY, ASTROPHYSICS AND COSMOLOGY.</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
    <subfield code="a">Christensen-Dalsgaard, J.</subfield>
    <subfield code="e">author.</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
    <subfield code="a">Kurtz, D. W.</subfield>
    <subfield code="e">author.</subfield>
  </datafield>
  <datafield tag="710" ind1="2" ind2=" ">
    <subfield code="a">SpringerLink (Online service)</subfield>
  </datafield>
  <datafield tag="773" ind1="0" ind2=" ">
    <subfield code="t">Springer eBooks</subfield>
  </datafield>
  <datafield tag="776" ind1="0" ind2="8">
    <subfield code="i">Printed edition:</subfield>
    <subfield code="z">9781402051784</subfield>
  </datafield>
  <datafield tag="830" ind1=" " ind2="0">
    <subfield code="a">Astronomy and Astrophysics Library,</subfield>
    <subfield code="x">0941-7834</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2="0">
    <subfield code="u">http://dx.doi.org/10.1007/978-1-4020-5803-5</subfield>
    <subfield code="z">Ver el texto completo en las instalaciones del CICY</subfield>
  </datafield>
  <datafield tag="912" ind1=" " ind2=" ">
    <subfield code="a">ZDB-2-PHA</subfield>
  </datafield>
  <datafield tag="942" ind1=" " ind2=" ">
    <subfield code="2">ddc</subfield>
    <subfield code="c">ER</subfield>
  </datafield>
  <datafield tag="999" ind1=" " ind2=" ">
    <subfield code="c">37375</subfield>
    <subfield code="d">37375</subfield>
  </datafield>
  <datafield tag="952" ind1=" " ind2=" ">
    <subfield code="0">0</subfield>
    <subfield code="1">0</subfield>
    <subfield code="2">ddc</subfield>
    <subfield code="4">0</subfield>
    <subfield code="7">0</subfield>
    <subfield code="8">LE</subfield>
    <subfield code="a">CICY</subfield>
    <subfield code="b">CICY</subfield>
    <subfield code="c">EL</subfield>
    <subfield code="d">2025-10-06</subfield>
    <subfield code="l">0</subfield>
    <subfield code="o">520</subfield>
    <subfield code="r">2025-10-06 08:45:26</subfield>
    <subfield code="w">2025-10-06</subfield>
    <subfield code="y">ER</subfield>
  </datafield>
</record>
