Advances in Helio- and Asteroseismology: Proceedings of the 123th Symposium of the International Astronomical Union, Held in Aarhus, Denmark, July 7–11, 1986
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1988
|
| Schriftenreihe: | International Astronomical Union / Union Astronomique Internationale
123 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | Helio- and asteroseismology study the interior of the Sun and other stars, by means of observations of oscillations on their surfaces. The last 10 years in the study of the solar interior, to a has witnessed a very rapid evolution point where we can now contemplate investigating the physical state of matter, or the details of rotation and other large-scale motion, in the Sun. The stellar studies are in some respects at the point of the solar studies 10 years ago, but appear poised to take off. Thus the time was deemed ripe for lAO Symposium No 123, to assess the present status of this work, and plan for its future development. Apart from the seismic data, few observations are available to provide information about stellar interiors. Detailed studies, by spectral analysis, can be made of stellar surface properties, including atmospheric temperature and chemical composition. However, the stellar radiative spectrum is almost entirely fixed by the mass, luminosity, radius and surface rotation of the star, and contains essentially no other information about the interior. An important test of stellar evolution theory is provided by observations of stel lar clusters, whose members can reasonably be assumed to have the same age and chemical composition. The location of such stars in a HR diagram, where luminosity is plotted against the effective temperature, can roughly be understood in terms of stellar evolution calculations |
| Beschreibung: | 1 Online-Ressource (628p) |
| ISBN: | 9789400940093 9789027726155 |
| DOI: | 10.1007/978-94-009-4009-3 |
Internformat
MARC
| LEADER | 00000nmm a2200000zcb4500 | ||
|---|---|---|---|
| 001 | BV042415142 | ||
| 003 | DE-604 | ||
| 005 | 20160609 | ||
| 007 | cr|uuu---uuuuu | ||
| 008 | 150316s1988 |||| o||u| ||||||eng d | ||
| 020 | |a 9789400940093 |c Online |9 978-94-009-4009-3 | ||
| 020 | |a 9789027726155 |c Print |9 978-90-277-2615-5 | ||
| 024 | 7 | |a 10.1007/978-94-009-4009-3 |2 doi | |
| 035 | |a (OCoLC)905376561 | ||
| 035 | |a (DE-599)BVBBV042415142 | ||
| 040 | |a DE-604 |b ger |e aacr | ||
| 041 | 0 | |a eng | |
| 049 | |a DE-91 |a DE-83 | ||
| 082 | 0 | |a 523.01 |2 23 | |
| 084 | |a PHY 000 |2 stub | ||
| 100 | 1 | |a Christensen-Dalsgaard, Jørgen |d 1950- |e Verfasser |0 (DE-588)131650297 |4 aut | |
| 245 | 1 | 0 | |a Advances in Helio- and Asteroseismology |b Proceedings of the 123th Symposium of the International Astronomical Union, Held in Aarhus, Denmark, July 7–11, 1986 |c edited by Jørgen Christensen-Dalsgaard, Søren Frandsen |
| 246 | 1 | 3 | |a Proceedings of the 123rd Symposium of the International Astromonomical Union, held in Aarhus, Denmark, July 7-11, 1986 |
| 264 | 1 | |a Dordrecht |b Springer Netherlands |c 1988 | |
| 300 | |a 1 Online-Ressource (628p) | ||
| 336 | |b txt |2 rdacontent | ||
| 337 | |b c |2 rdamedia | ||
| 338 | |b cr |2 rdacarrier | ||
| 490 | 0 | |a International Astronomical Union / Union Astronomique Internationale |v 123 | |
| 500 | |a Helio- and asteroseismology study the interior of the Sun and other stars, by means of observations of oscillations on their surfaces. The last 10 years in the study of the solar interior, to a has witnessed a very rapid evolution point where we can now contemplate investigating the physical state of matter, or the details of rotation and other large-scale motion, in the Sun. The stellar studies are in some respects at the point of the solar studies 10 years ago, but appear poised to take off. Thus the time was deemed ripe for lAO Symposium No 123, to assess the present status of this work, and plan for its future development. Apart from the seismic data, few observations are available to provide information about stellar interiors. Detailed studies, by spectral analysis, can be made of stellar surface properties, including atmospheric temperature and chemical composition. However, the stellar radiative spectrum is almost entirely fixed by the mass, luminosity, radius and surface rotation of the star, and contains essentially no other information about the interior. An important test of stellar evolution theory is provided by observations of stel lar clusters, whose members can reasonably be assumed to have the same age and chemical composition. The location of such stars in a HR diagram, where luminosity is plotted against the effective temperature, can roughly be understood in terms of stellar evolution calculations | ||
| 650 | 4 | |a Physics | |
| 650 | 4 | |a Astrophysics and Astroparticles | |
| 650 | 0 | 7 | |a Stern |0 (DE-588)4057342-4 |2 gnd |9 rswk-swf |
| 650 | 0 | 7 | |a Seismologie |0 (DE-588)4379341-1 |2 gnd |9 rswk-swf |
| 651 | 7 | |a Sonne |0 (DE-588)1236963652 |2 gnd |9 rswk-swf | |
| 655 | 7 | |8 1\p |0 (DE-588)1071861417 |a Konferenzschrift |y 1986 |z Århus |2 gnd-content | |
| 689 | 0 | 0 | |a Seismologie |0 (DE-588)4379341-1 |D s |
| 689 | 0 | 1 | |a Stern |0 (DE-588)4057342-4 |D s |
| 689 | 0 | |8 2\p |5 DE-604 | |
| 689 | 1 | 0 | |a Seismologie |0 (DE-588)4379341-1 |D s |
| 689 | 1 | 1 | |a Sonne |0 (DE-588)1236963652 |D g |
| 689 | 1 | |8 3\p |5 DE-604 | |
| 700 | 1 | |a Frandsen, Søren |d 1946- |e Sonstige |0 (DE-588)1096254751 |4 oth | |
| 856 | 4 | 0 | |u https://doi.org/10.1007/978-94-009-4009-3 |x Verlag |3 Volltext |
| 912 | |a ZDB-2-PHA |a ZDB-2-BAE | ||
| 940 | 1 | |q ZDB-2-PHA_Archive | |
| 999 | |a oai:aleph.bib-bvb.de:BVB01-027850635 | ||
| 883 | 1 | |8 1\p |a cgwrk |d 20201028 |q DE-101 |u https://d-nb.info/provenance/plan#cgwrk | |
| 883 | 1 | |8 2\p |a cgwrk |d 20201028 |q DE-101 |u https://d-nb.info/provenance/plan#cgwrk | |
| 883 | 1 | |8 3\p |a cgwrk |d 20201028 |q DE-101 |u https://d-nb.info/provenance/plan#cgwrk | |
Datensatz im Suchindex
| _version_ | 1804153081822183424 |
|---|---|
| any_adam_object | |
| author | Christensen-Dalsgaard, Jørgen 1950- |
| author_GND | (DE-588)131650297 (DE-588)1096254751 |
| author_facet | Christensen-Dalsgaard, Jørgen 1950- |
| author_role | aut |
| author_sort | Christensen-Dalsgaard, Jørgen 1950- |
| author_variant | j c d jcd |
| building | Verbundindex |
| bvnumber | BV042415142 |
| classification_tum | PHY 000 |
| collection | ZDB-2-PHA ZDB-2-BAE |
| ctrlnum | (OCoLC)905376561 (DE-599)BVBBV042415142 |
| dewey-full | 523.01 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.01 |
| dewey-search | 523.01 |
| dewey-sort | 3523.01 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1007/978-94-009-4009-3 |
| format | Electronic eBook |
| fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>03855nmm a2200565zcb4500</leader><controlfield tag="001">BV042415142</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">20160609 </controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">150316s1988 |||| o||u| ||||||eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9789400940093</subfield><subfield code="c">Online</subfield><subfield code="9">978-94-009-4009-3</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9789027726155</subfield><subfield code="c">Print</subfield><subfield code="9">978-90-277-2615-5</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/978-94-009-4009-3</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)905376561</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV042415142</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-604</subfield><subfield code="b">ger</subfield><subfield code="e">aacr</subfield></datafield><datafield tag="041" ind1="0" ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="049" ind1=" " ind2=" "><subfield code="a">DE-91</subfield><subfield code="a">DE-83</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">523.01</subfield><subfield code="2">23</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">PHY 000</subfield><subfield code="2">stub</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Christensen-Dalsgaard, Jørgen</subfield><subfield code="d">1950-</subfield><subfield code="e">Verfasser</subfield><subfield code="0">(DE-588)131650297</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Advances in Helio- and Asteroseismology</subfield><subfield code="b">Proceedings of the 123th Symposium of the International Astronomical Union, Held in Aarhus, Denmark, July 7–11, 1986</subfield><subfield code="c">edited by Jørgen Christensen-Dalsgaard, Søren Frandsen</subfield></datafield><datafield tag="246" ind1="1" ind2="3"><subfield code="a">Proceedings of the 123rd Symposium of the International Astromonomical Union, held in Aarhus, Denmark, July 7-11, 1986</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Dordrecht</subfield><subfield code="b">Springer Netherlands</subfield><subfield code="c">1988</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 Online-Ressource (628p)</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="490" ind1="0" ind2=" "><subfield code="a">International Astronomical Union / Union Astronomique Internationale</subfield><subfield code="v">123</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">Helio- and asteroseismology study the interior of the Sun and other stars, by means of observations of oscillations on their surfaces. The last 10 years in the study of the solar interior, to a has witnessed a very rapid evolution point where we can now contemplate investigating the physical state of matter, or the details of rotation and other large-scale motion, in the Sun. The stellar studies are in some respects at the point of the solar studies 10 years ago, but appear poised to take off. Thus the time was deemed ripe for lAO Symposium No 123, to assess the present status of this work, and plan for its future development. Apart from the seismic data, few observations are available to provide information about stellar interiors. Detailed studies, by spectral analysis, can be made of stellar surface properties, including atmospheric temperature and chemical composition. However, the stellar radiative spectrum is almost entirely fixed by the mass, luminosity, radius and surface rotation of the star, and contains essentially no other information about the interior. An important test of stellar evolution theory is provided by observations of stel lar clusters, whose members can reasonably be assumed to have the same age and chemical composition. The location of such stars in a HR diagram, where luminosity is plotted against the effective temperature, can roughly be understood in terms of stellar evolution calculations</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Physics</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Astrophysics and Astroparticles</subfield></datafield><datafield tag="650" ind1="0" ind2="7"><subfield code="a">Stern</subfield><subfield code="0">(DE-588)4057342-4</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="650" ind1="0" ind2="7"><subfield code="a">Seismologie</subfield><subfield code="0">(DE-588)4379341-1</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="651" ind1=" " ind2="7"><subfield code="a">Sonne</subfield><subfield code="0">(DE-588)1236963652</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="655" ind1=" " ind2="7"><subfield code="8">1\p</subfield><subfield code="0">(DE-588)1071861417</subfield><subfield code="a">Konferenzschrift</subfield><subfield code="y">1986</subfield><subfield code="z">Århus</subfield><subfield code="2">gnd-content</subfield></datafield><datafield tag="689" ind1="0" ind2="0"><subfield code="a">Seismologie</subfield><subfield code="0">(DE-588)4379341-1</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="0" ind2="1"><subfield code="a">Stern</subfield><subfield code="0">(DE-588)4057342-4</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="0" ind2=" "><subfield code="8">2\p</subfield><subfield code="5">DE-604</subfield></datafield><datafield tag="689" ind1="1" ind2="0"><subfield code="a">Seismologie</subfield><subfield code="0">(DE-588)4379341-1</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="1" ind2="1"><subfield code="a">Sonne</subfield><subfield code="0">(DE-588)1236963652</subfield><subfield code="D">g</subfield></datafield><datafield tag="689" ind1="1" ind2=" "><subfield code="8">3\p</subfield><subfield code="5">DE-604</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Frandsen, Søren</subfield><subfield code="d">1946-</subfield><subfield code="e">Sonstige</subfield><subfield code="0">(DE-588)1096254751</subfield><subfield code="4">oth</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1007/978-94-009-4009-3</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-2-PHA</subfield><subfield code="a">ZDB-2-BAE</subfield></datafield><datafield tag="940" ind1="1" ind2=" "><subfield code="q">ZDB-2-PHA_Archive</subfield></datafield><datafield tag="999" ind1=" " ind2=" "><subfield code="a">oai:aleph.bib-bvb.de:BVB01-027850635</subfield></datafield><datafield tag="883" ind1="1" ind2=" "><subfield code="8">1\p</subfield><subfield code="a">cgwrk</subfield><subfield code="d">20201028</subfield><subfield code="q">DE-101</subfield><subfield code="u">https://d-nb.info/provenance/plan#cgwrk</subfield></datafield><datafield tag="883" ind1="1" ind2=" "><subfield code="8">2\p</subfield><subfield code="a">cgwrk</subfield><subfield code="d">20201028</subfield><subfield code="q">DE-101</subfield><subfield code="u">https://d-nb.info/provenance/plan#cgwrk</subfield></datafield><datafield tag="883" ind1="1" ind2=" "><subfield code="8">3\p</subfield><subfield code="a">cgwrk</subfield><subfield code="d">20201028</subfield><subfield code="q">DE-101</subfield><subfield code="u">https://d-nb.info/provenance/plan#cgwrk</subfield></datafield></record></collection> |
| genre | 1\p (DE-588)1071861417 Konferenzschrift 1986 Århus gnd-content |
| genre_facet | Konferenzschrift 1986 Århus |
| geographic | Sonne (DE-588)1236963652 gnd |
| geographic_facet | Sonne |
| id | DE-604.BV042415142 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:56Z |
| institution | BVB |
| isbn | 9789400940093 9789027726155 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-027850635 |
| oclc_num | 905376561 |
| open_access_boolean | |
| owner | DE-91 DE-BY-TUM DE-83 |
| owner_facet | DE-91 DE-BY-TUM DE-83 |
| physical | 1 Online-Ressource (628p) |
| psigel | ZDB-2-PHA ZDB-2-BAE ZDB-2-PHA_Archive |
| publishDate | 1988 |
| publishDateSearch | 1988 |
| publishDateSort | 1988 |
| publisher | Springer Netherlands |
| record_format | marc |
| series2 | International Astronomical Union / Union Astronomique Internationale |
| spelling | Christensen-Dalsgaard, Jørgen 1950- Verfasser (DE-588)131650297 aut Advances in Helio- and Asteroseismology Proceedings of the 123th Symposium of the International Astronomical Union, Held in Aarhus, Denmark, July 7–11, 1986 edited by Jørgen Christensen-Dalsgaard, Søren Frandsen Proceedings of the 123rd Symposium of the International Astromonomical Union, held in Aarhus, Denmark, July 7-11, 1986 Dordrecht Springer Netherlands 1988 1 Online-Ressource (628p) txt rdacontent c rdamedia cr rdacarrier International Astronomical Union / Union Astronomique Internationale 123 Helio- and asteroseismology study the interior of the Sun and other stars, by means of observations of oscillations on their surfaces. The last 10 years in the study of the solar interior, to a has witnessed a very rapid evolution point where we can now contemplate investigating the physical state of matter, or the details of rotation and other large-scale motion, in the Sun. The stellar studies are in some respects at the point of the solar studies 10 years ago, but appear poised to take off. Thus the time was deemed ripe for lAO Symposium No 123, to assess the present status of this work, and plan for its future development. Apart from the seismic data, few observations are available to provide information about stellar interiors. Detailed studies, by spectral analysis, can be made of stellar surface properties, including atmospheric temperature and chemical composition. However, the stellar radiative spectrum is almost entirely fixed by the mass, luminosity, radius and surface rotation of the star, and contains essentially no other information about the interior. An important test of stellar evolution theory is provided by observations of stel lar clusters, whose members can reasonably be assumed to have the same age and chemical composition. The location of such stars in a HR diagram, where luminosity is plotted against the effective temperature, can roughly be understood in terms of stellar evolution calculations Physics Astrophysics and Astroparticles Stern (DE-588)4057342-4 gnd rswk-swf Seismologie (DE-588)4379341-1 gnd rswk-swf Sonne (DE-588)1236963652 gnd rswk-swf 1\p (DE-588)1071861417 Konferenzschrift 1986 Århus gnd-content Seismologie (DE-588)4379341-1 s Stern (DE-588)4057342-4 s 2\p DE-604 Sonne (DE-588)1236963652 g 3\p DE-604 Frandsen, Søren 1946- Sonstige (DE-588)1096254751 oth https://doi.org/10.1007/978-94-009-4009-3 Verlag Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 2\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 3\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Christensen-Dalsgaard, Jørgen 1950- Advances in Helio- and Asteroseismology Proceedings of the 123th Symposium of the International Astronomical Union, Held in Aarhus, Denmark, July 7–11, 1986 Physics Astrophysics and Astroparticles Stern (DE-588)4057342-4 gnd Seismologie (DE-588)4379341-1 gnd |
| subject_GND | (DE-588)4057342-4 (DE-588)4379341-1 (DE-588)1236963652 (DE-588)1071861417 |
| title | Advances in Helio- and Asteroseismology Proceedings of the 123th Symposium of the International Astronomical Union, Held in Aarhus, Denmark, July 7–11, 1986 |
| title_alt | Proceedings of the 123rd Symposium of the International Astromonomical Union, held in Aarhus, Denmark, July 7-11, 1986 |
| title_auth | Advances in Helio- and Asteroseismology Proceedings of the 123th Symposium of the International Astronomical Union, Held in Aarhus, Denmark, July 7–11, 1986 |
| title_exact_search | Advances in Helio- and Asteroseismology Proceedings of the 123th Symposium of the International Astronomical Union, Held in Aarhus, Denmark, July 7–11, 1986 |
| title_full | Advances in Helio- and Asteroseismology Proceedings of the 123th Symposium of the International Astronomical Union, Held in Aarhus, Denmark, July 7–11, 1986 edited by Jørgen Christensen-Dalsgaard, Søren Frandsen |
| title_fullStr | Advances in Helio- and Asteroseismology Proceedings of the 123th Symposium of the International Astronomical Union, Held in Aarhus, Denmark, July 7–11, 1986 edited by Jørgen Christensen-Dalsgaard, Søren Frandsen |
| title_full_unstemmed | Advances in Helio- and Asteroseismology Proceedings of the 123th Symposium of the International Astronomical Union, Held in Aarhus, Denmark, July 7–11, 1986 edited by Jørgen Christensen-Dalsgaard, Søren Frandsen |
| title_short | Advances in Helio- and Asteroseismology |
| title_sort | advances in helio and asteroseismology proceedings of the 123th symposium of the international astronomical union held in aarhus denmark july 7 11 1986 |
| title_sub | Proceedings of the 123th Symposium of the International Astronomical Union, Held in Aarhus, Denmark, July 7–11, 1986 |
| topic | Physics Astrophysics and Astroparticles Stern (DE-588)4057342-4 gnd Seismologie (DE-588)4379341-1 gnd |
| topic_facet | Physics Astrophysics and Astroparticles Stern Seismologie Sonne Konferenzschrift 1986 Århus |
| url | https://doi.org/10.1007/978-94-009-4009-3 |
| work_keys_str_mv | AT christensendalsgaardjørgen advancesinhelioandasteroseismologyproceedingsofthe123thsymposiumoftheinternationalastronomicalunionheldinaarhusdenmarkjuly7111986 AT frandsensøren advancesinhelioandasteroseismologyproceedingsofthe123thsymposiumoftheinternationalastronomicalunionheldinaarhusdenmarkjuly7111986 AT christensendalsgaardjørgen proceedingsofthe123rdsymposiumoftheinternationalastromonomicalunionheldinaarhusdenmarkjuly7111986 AT frandsensøren proceedingsofthe123rdsymposiumoftheinternationalastromonomicalunionheldinaarhusdenmarkjuly7111986 |