The Brightest Stars:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1980
|
| Schriftenreihe: | Geophysics and Astrophysics Monographs, An International Series of Fundamental Textbooks
19 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | No part of the Hertzsprung-Russell diagram shows a more pronounced diversity of stellar types than the upper part, which contains the most luminous stars. Can one visualize a larger difference than between a luminous, young and extremely hot Of star, and a cool, evolved pulsating giant of the Mira type, or an S-type supergiant, or - again at the other side of the diagram - the compact nucleus of a planetary nebula? But there is order and unity in this apparent disorder! Virtually all types of bright stars are evolutionally related, in one way or the other. Evolution links bright stars. In many cases the evolution is speeded up by, or at least intimately related to various signs of stellar instability. Bright stars lose mass, either continuously or in dramatic sudden events, they vibrate or pulsate - and with these tenuous, gigantic objects this often happens in a most bizarre fashion. Sometimes the evolution goes so fast that fundamental changes are observable in the time span of a human's life - several of such cases have now been identified |
| Beschreibung: | 1 Online-Ressource (470p) |
| ISBN: | 9789400990302 9789027711106 |
| DOI: | 10.1007/978-94-009-9030-2 |
Internformat
MARC
| LEADER | 00000nmm a2200000zcb4500 | ||
|---|---|---|---|
| 001 | BV042415432 | ||
| 003 | DE-604 | ||
| 005 | 20210530 | ||
| 007 | cr|uuu---uuuuu | ||
| 008 | 150316s1980 |||| o||u| ||||||eng d | ||
| 020 | |a 9789400990302 |c Online |9 978-94-009-9030-2 | ||
| 020 | |a 9789027711106 |c Print |9 978-90-277-1110-6 | ||
| 024 | 7 | |a 10.1007/978-94-009-9030-2 |2 doi | |
| 035 | |a (OCoLC)863785158 | ||
| 035 | |a (DE-599)BVBBV042415432 | ||
| 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 Jager, Cornelis de |d 1921-2021 |e Verfasser |0 (DE-588)127810188 |4 aut | |
| 245 | 1 | 0 | |a The Brightest Stars |c by Cornelis Jager |
| 264 | 1 | |a Dordrecht |b Springer Netherlands |c 1980 | |
| 300 | |a 1 Online-Ressource (470p) | ||
| 336 | |b txt |2 rdacontent | ||
| 337 | |b c |2 rdamedia | ||
| 338 | |b cr |2 rdacarrier | ||
| 490 | 0 | |a Geophysics and Astrophysics Monographs, An International Series of Fundamental Textbooks |v 19 | |
| 500 | |a No part of the Hertzsprung-Russell diagram shows a more pronounced diversity of stellar types than the upper part, which contains the most luminous stars. Can one visualize a larger difference than between a luminous, young and extremely hot Of star, and a cool, evolved pulsating giant of the Mira type, or an S-type supergiant, or - again at the other side of the diagram - the compact nucleus of a planetary nebula? But there is order and unity in this apparent disorder! Virtually all types of bright stars are evolutionally related, in one way or the other. Evolution links bright stars. In many cases the evolution is speeded up by, or at least intimately related to various signs of stellar instability. Bright stars lose mass, either continuously or in dramatic sudden events, they vibrate or pulsate - and with these tenuous, gigantic objects this often happens in a most bizarre fashion. Sometimes the evolution goes so fast that fundamental changes are observable in the time span of a human's life - several of such cases have now been identified | ||
| 650 | 4 | |a Physics | |
| 650 | 4 | |a Astrophysics and Astroparticles | |
| 650 | 0 | 7 | |a Nova |0 (DE-588)4172093-3 |2 gnd |9 rswk-swf |
| 650 | 0 | 7 | |a Helligkeit |0 (DE-588)4226160-0 |2 gnd |9 rswk-swf |
| 650 | 0 | 7 | |a Stern |0 (DE-588)4057342-4 |2 gnd |9 rswk-swf |
| 689 | 0 | 0 | |a Stern |0 (DE-588)4057342-4 |D s |
| 689 | 0 | 1 | |a Helligkeit |0 (DE-588)4226160-0 |D s |
| 689 | 0 | |8 1\p |5 DE-604 | |
| 689 | 1 | 0 | |a Nova |0 (DE-588)4172093-3 |D s |
| 689 | 1 | |8 2\p |5 DE-604 | |
| 856 | 4 | 0 | |u https://doi.org/10.1007/978-94-009-9030-2 |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:BVB01-027850925 | ||
| 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 | |
Datensatz im Suchindex
| _version_ | 1804153082494320640 |
|---|---|
| any_adam_object | |
| author | Jager, Cornelis de 1921-2021 |
| author_GND | (DE-588)127810188 |
| author_facet | Jager, Cornelis de 1921-2021 |
| author_role | aut |
| author_sort | Jager, Cornelis de 1921-2021 |
| author_variant | c d j cd cdj |
| building | Verbundindex |
| bvnumber | BV042415432 |
| classification_tum | PHY 000 |
| collection | ZDB-2-PHA ZDB-2-BAE |
| ctrlnum | (OCoLC)863785158 (DE-599)BVBBV042415432 |
| 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 | 10.1007/978-94-009-9030-2 |
| format | Electronic eBook |
| fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>02869nmm a2200505zcb4500</leader><controlfield tag="001">BV042415432</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">20210530 </controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">150316s1980 |||| o||u| ||||||eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9789400990302</subfield><subfield code="c">Online</subfield><subfield code="9">978-94-009-9030-2</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9789027711106</subfield><subfield code="c">Print</subfield><subfield code="9">978-90-277-1110-6</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/978-94-009-9030-2</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)863785158</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV042415432</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">Jager, Cornelis de</subfield><subfield code="d">1921-2021</subfield><subfield code="e">Verfasser</subfield><subfield code="0">(DE-588)127810188</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">The Brightest Stars</subfield><subfield code="c">by Cornelis Jager</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Dordrecht</subfield><subfield code="b">Springer Netherlands</subfield><subfield code="c">1980</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 Online-Ressource (470p)</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">Geophysics and Astrophysics Monographs, An International Series of Fundamental Textbooks</subfield><subfield code="v">19</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">No part of the Hertzsprung-Russell diagram shows a more pronounced diversity of stellar types than the upper part, which contains the most luminous stars. Can one visualize a larger difference than between a luminous, young and extremely hot Of star, and a cool, evolved pulsating giant of the Mira type, or an S-type supergiant, or - again at the other side of the diagram - the compact nucleus of a planetary nebula? But there is order and unity in this apparent disorder! Virtually all types of bright stars are evolutionally related, in one way or the other. Evolution links bright stars. In many cases the evolution is speeded up by, or at least intimately related to various signs of stellar instability. Bright stars lose mass, either continuously or in dramatic sudden events, they vibrate or pulsate - and with these tenuous, gigantic objects this often happens in a most bizarre fashion. Sometimes the evolution goes so fast that fundamental changes are observable in the time span of a human's life - several of such cases have now been identified</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">Nova</subfield><subfield code="0">(DE-588)4172093-3</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="650" ind1="0" ind2="7"><subfield code="a">Helligkeit</subfield><subfield code="0">(DE-588)4226160-0</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</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="689" ind1="0" ind2="0"><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="1"><subfield code="a">Helligkeit</subfield><subfield code="0">(DE-588)4226160-0</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="0" ind2=" "><subfield code="8">1\p</subfield><subfield code="5">DE-604</subfield></datafield><datafield tag="689" ind1="1" ind2="0"><subfield code="a">Nova</subfield><subfield code="0">(DE-588)4172093-3</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="1" ind2=" "><subfield code="8">2\p</subfield><subfield code="5">DE-604</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1007/978-94-009-9030-2</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:BVB01-027850925</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></record></collection> |
| id | DE-604.BV042415432 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:57Z |
| institution | BVB |
| isbn | 9789400990302 9789027711106 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-027850925 |
| oclc_num | 863785158 |
| open_access_boolean | |
| owner | DE-91 DE-BY-TUM DE-83 |
| owner_facet | DE-91 DE-BY-TUM DE-83 |
| physical | 1 Online-Ressource (470p) |
| psigel | ZDB-2-PHA ZDB-2-BAE ZDB-2-PHA_Archive |
| publishDate | 1980 |
| publishDateSearch | 1980 |
| publishDateSort | 1980 |
| publisher | Springer Netherlands |
| record_format | marc |
| series2 | Geophysics and Astrophysics Monographs, An International Series of Fundamental Textbooks |
| spelling | Jager, Cornelis de 1921-2021 Verfasser (DE-588)127810188 aut The Brightest Stars by Cornelis Jager Dordrecht Springer Netherlands 1980 1 Online-Ressource (470p) txt rdacontent c rdamedia cr rdacarrier Geophysics and Astrophysics Monographs, An International Series of Fundamental Textbooks 19 No part of the Hertzsprung-Russell diagram shows a more pronounced diversity of stellar types than the upper part, which contains the most luminous stars. Can one visualize a larger difference than between a luminous, young and extremely hot Of star, and a cool, evolved pulsating giant of the Mira type, or an S-type supergiant, or - again at the other side of the diagram - the compact nucleus of a planetary nebula? But there is order and unity in this apparent disorder! Virtually all types of bright stars are evolutionally related, in one way or the other. Evolution links bright stars. In many cases the evolution is speeded up by, or at least intimately related to various signs of stellar instability. Bright stars lose mass, either continuously or in dramatic sudden events, they vibrate or pulsate - and with these tenuous, gigantic objects this often happens in a most bizarre fashion. Sometimes the evolution goes so fast that fundamental changes are observable in the time span of a human's life - several of such cases have now been identified Physics Astrophysics and Astroparticles Nova (DE-588)4172093-3 gnd rswk-swf Helligkeit (DE-588)4226160-0 gnd rswk-swf Stern (DE-588)4057342-4 gnd rswk-swf Stern (DE-588)4057342-4 s Helligkeit (DE-588)4226160-0 s 1\p DE-604 Nova (DE-588)4172093-3 s 2\p DE-604 https://doi.org/10.1007/978-94-009-9030-2 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 |
| spellingShingle | Jager, Cornelis de 1921-2021 The Brightest Stars Physics Astrophysics and Astroparticles Nova (DE-588)4172093-3 gnd Helligkeit (DE-588)4226160-0 gnd Stern (DE-588)4057342-4 gnd |
| subject_GND | (DE-588)4172093-3 (DE-588)4226160-0 (DE-588)4057342-4 |
| title | The Brightest Stars |
| title_auth | The Brightest Stars |
| title_exact_search | The Brightest Stars |
| title_full | The Brightest Stars by Cornelis Jager |
| title_fullStr | The Brightest Stars by Cornelis Jager |
| title_full_unstemmed | The Brightest Stars by Cornelis Jager |
| title_short | The Brightest Stars |
| title_sort | the brightest stars |
| topic | Physics Astrophysics and Astroparticles Nova (DE-588)4172093-3 gnd Helligkeit (DE-588)4226160-0 gnd Stern (DE-588)4057342-4 gnd |
| topic_facet | Physics Astrophysics and Astroparticles Nova Helligkeit Stern |
| url | https://doi.org/10.1007/978-94-009-9030-2 |
| work_keys_str_mv | AT jagercornelisde thebrighteststars |