Timing Neutron Stars:
Gespeichert in:
1. Verfasser: | |
---|---|
Format: | Elektronisch E-Book |
Sprache: | English |
Veröffentlicht: |
Dordrecht
Springer Netherlands
1989
|
Schriftenreihe: | NATO ASI Series, Series C: Mathematical and Physical Sciences
262 |
Schlagworte: | |
Online-Zugang: | Volltext |
Beschreibung: | The idea for organizing an Advanced Study Institute devoted largely to neutron star timing arose independently in three places, at Istanbul, Garching and Amster dam; when we became aware of each other's ideas we decided to join forces. The choice of a place for the Institute, in Turkey, appealed much to us all, and it was then quickly decided that Qe§me would be an excellent spot. When the preparations for the Institute started, early in 1987, we could not have guessed how timely the subject actually was. Of course, the recently dis covered QPO phenomena in accreting neutron stars and half a dozen binary and millisecond radio pulsars known at the time formed one of the basic motivations for organizing this Institute. But none of us could have guessed that later in 1987 we were to witness the wonderful discovery of the binary and millisecond radio pulsars in globular clusters and, -as if Nature wished to give us a special present for this the discovery in March 1988 of a millisecond pulsar in an eclipsing binary Institu- system, the first eclipsing radio pulsar ever found, and the second fastest in the sky! The discussion of this pulsar, its formation and fate was one of the highlights of this meeting, especially since its discoverers were among the participants of the Institute and could provide us with first-hand information |
Beschreibung: | 1 Online-Ressource (XVIII, 774 p) |
ISBN: | 9789400922730 9789401075190 |
ISSN: | 1389-2185 |
DOI: | 10.1007/978-94-009-2273-0 |
Internformat
MARC
LEADER | 00000nmm a2200000zcb4500 | ||
---|---|---|---|
001 | BV042415004 | ||
003 | DE-604 | ||
005 | 00000000000000.0 | ||
007 | cr|uuu---uuuuu | ||
008 | 150316s1989 |||| o||u| ||||||eng d | ||
020 | |a 9789400922730 |c Online |9 978-94-009-2273-0 | ||
020 | |a 9789401075190 |c Print |9 978-94-010-7519-0 | ||
024 | 7 | |a 10.1007/978-94-009-2273-0 |2 doi | |
035 | |a (OCoLC)906736008 | ||
035 | |a (DE-599)BVBBV042415004 | ||
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 Ögelman, H. |e Verfasser |4 aut | |
245 | 1 | 0 | |a Timing Neutron Stars |c edited by H. Ögelman, E. P. J. Heuvel |
246 | 1 | 3 | |a Proceedings of the NATO Advanced Study Institute, Çesme, Izmir, Turkey, 4-15 April 1988 |
264 | 1 | |a Dordrecht |b Springer Netherlands |c 1989 | |
300 | |a 1 Online-Ressource (XVIII, 774 p) | ||
336 | |b txt |2 rdacontent | ||
337 | |b c |2 rdamedia | ||
338 | |b cr |2 rdacarrier | ||
490 | 0 | |a NATO ASI Series, Series C: Mathematical and Physical Sciences |v 262 |x 1389-2185 | |
500 | |a The idea for organizing an Advanced Study Institute devoted largely to neutron star timing arose independently in three places, at Istanbul, Garching and Amster dam; when we became aware of each other's ideas we decided to join forces. The choice of a place for the Institute, in Turkey, appealed much to us all, and it was then quickly decided that Qe§me would be an excellent spot. When the preparations for the Institute started, early in 1987, we could not have guessed how timely the subject actually was. Of course, the recently dis covered QPO phenomena in accreting neutron stars and half a dozen binary and millisecond radio pulsars known at the time formed one of the basic motivations for organizing this Institute. But none of us could have guessed that later in 1987 we were to witness the wonderful discovery of the binary and millisecond radio pulsars in globular clusters and, -as if Nature wished to give us a special present for this the discovery in March 1988 of a millisecond pulsar in an eclipsing binary Institu- system, the first eclipsing radio pulsar ever found, and the second fastest in the sky! The discussion of this pulsar, its formation and fate was one of the highlights of this meeting, especially since its discoverers were among the participants of the Institute and could provide us with first-hand information | ||
650 | 4 | |a Physics | |
650 | 4 | |a Astrophysics and Astroparticles | |
650 | 4 | |a Statistics for Engineering, Physics, Computer Science, Chemistry and Earth Sciences | |
700 | 1 | |a Heuvel, E. P. J. |e Sonstige |4 oth | |
856 | 4 | 0 | |u https://doi.org/10.1007/978-94-009-2273-0 |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:BVB01-027850497 |
Datensatz im Suchindex
_version_ | 1804153081496076288 |
---|---|
any_adam_object | |
author | Ögelman, H. |
author_facet | Ögelman, H. |
author_role | aut |
author_sort | Ögelman, H. |
author_variant | h ö hö |
building | Verbundindex |
bvnumber | BV042415004 |
classification_tum | PHY 000 |
collection | ZDB-2-PHA ZDB-2-BAE |
ctrlnum | (OCoLC)906736008 (DE-599)BVBBV042415004 |
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 | 10.1007/978-94-009-2273-0 |
format | Electronic eBook |
fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>02855nmm a2200421zcb4500</leader><controlfield tag="001">BV042415004</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">00000000000000.0</controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">150316s1989 |||| o||u| ||||||eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9789400922730</subfield><subfield code="c">Online</subfield><subfield code="9">978-94-009-2273-0</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9789401075190</subfield><subfield code="c">Print</subfield><subfield code="9">978-94-010-7519-0</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/978-94-009-2273-0</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)906736008</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV042415004</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">Ögelman, H.</subfield><subfield code="e">Verfasser</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Timing Neutron Stars</subfield><subfield code="c">edited by H. Ögelman, E. P. J. Heuvel</subfield></datafield><datafield tag="246" ind1="1" ind2="3"><subfield code="a">Proceedings of the NATO Advanced Study Institute, Çesme, Izmir, Turkey, 4-15 April 1988</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Dordrecht</subfield><subfield code="b">Springer Netherlands</subfield><subfield code="c">1989</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 Online-Ressource (XVIII, 774 p)</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">NATO ASI Series, Series C: Mathematical and Physical Sciences</subfield><subfield code="v">262</subfield><subfield code="x">1389-2185</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">The idea for organizing an Advanced Study Institute devoted largely to neutron star timing arose independently in three places, at Istanbul, Garching and Amster dam; when we became aware of each other's ideas we decided to join forces. The choice of a place for the Institute, in Turkey, appealed much to us all, and it was then quickly decided that Qe§me would be an excellent spot. When the preparations for the Institute started, early in 1987, we could not have guessed how timely the subject actually was. Of course, the recently dis covered QPO phenomena in accreting neutron stars and half a dozen binary and millisecond radio pulsars known at the time formed one of the basic motivations for organizing this Institute. But none of us could have guessed that later in 1987 we were to witness the wonderful discovery of the binary and millisecond radio pulsars in globular clusters and, -as if Nature wished to give us a special present for this the discovery in March 1988 of a millisecond pulsar in an eclipsing binary Institu- system, the first eclipsing radio pulsar ever found, and the second fastest in the sky! The discussion of this pulsar, its formation and fate was one of the highlights of this meeting, especially since its discoverers were among the participants of the Institute and could provide us with first-hand information</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=" " ind2="4"><subfield code="a">Statistics for Engineering, Physics, Computer Science, Chemistry and Earth Sciences</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Heuvel, E. P. J.</subfield><subfield code="e">Sonstige</subfield><subfield code="4">oth</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1007/978-94-009-2273-0</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:BVB01-027850497</subfield></datafield></record></collection> |
id | DE-604.BV042415004 |
illustrated | Not Illustrated |
indexdate | 2024-07-10T01:20:56Z |
institution | BVB |
isbn | 9789400922730 9789401075190 |
issn | 1389-2185 |
language | English |
oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-027850497 |
oclc_num | 906736008 |
open_access_boolean | |
owner | DE-91 DE-BY-TUM DE-83 |
owner_facet | DE-91 DE-BY-TUM DE-83 |
physical | 1 Online-Ressource (XVIII, 774 p) |
psigel | ZDB-2-PHA ZDB-2-BAE ZDB-2-PHA_Archive |
publishDate | 1989 |
publishDateSearch | 1989 |
publishDateSort | 1989 |
publisher | Springer Netherlands |
record_format | marc |
series2 | NATO ASI Series, Series C: Mathematical and Physical Sciences |
spelling | Ögelman, H. Verfasser aut Timing Neutron Stars edited by H. Ögelman, E. P. J. Heuvel Proceedings of the NATO Advanced Study Institute, Çesme, Izmir, Turkey, 4-15 April 1988 Dordrecht Springer Netherlands 1989 1 Online-Ressource (XVIII, 774 p) txt rdacontent c rdamedia cr rdacarrier NATO ASI Series, Series C: Mathematical and Physical Sciences 262 1389-2185 The idea for organizing an Advanced Study Institute devoted largely to neutron star timing arose independently in three places, at Istanbul, Garching and Amster dam; when we became aware of each other's ideas we decided to join forces. The choice of a place for the Institute, in Turkey, appealed much to us all, and it was then quickly decided that Qe§me would be an excellent spot. When the preparations for the Institute started, early in 1987, we could not have guessed how timely the subject actually was. Of course, the recently dis covered QPO phenomena in accreting neutron stars and half a dozen binary and millisecond radio pulsars known at the time formed one of the basic motivations for organizing this Institute. But none of us could have guessed that later in 1987 we were to witness the wonderful discovery of the binary and millisecond radio pulsars in globular clusters and, -as if Nature wished to give us a special present for this the discovery in March 1988 of a millisecond pulsar in an eclipsing binary Institu- system, the first eclipsing radio pulsar ever found, and the second fastest in the sky! The discussion of this pulsar, its formation and fate was one of the highlights of this meeting, especially since its discoverers were among the participants of the Institute and could provide us with first-hand information Physics Astrophysics and Astroparticles Statistics for Engineering, Physics, Computer Science, Chemistry and Earth Sciences Heuvel, E. P. J. Sonstige oth https://doi.org/10.1007/978-94-009-2273-0 Verlag Volltext |
spellingShingle | Ögelman, H. Timing Neutron Stars Physics Astrophysics and Astroparticles Statistics for Engineering, Physics, Computer Science, Chemistry and Earth Sciences |
title | Timing Neutron Stars |
title_alt | Proceedings of the NATO Advanced Study Institute, Çesme, Izmir, Turkey, 4-15 April 1988 |
title_auth | Timing Neutron Stars |
title_exact_search | Timing Neutron Stars |
title_full | Timing Neutron Stars edited by H. Ögelman, E. P. J. Heuvel |
title_fullStr | Timing Neutron Stars edited by H. Ögelman, E. P. J. Heuvel |
title_full_unstemmed | Timing Neutron Stars edited by H. Ögelman, E. P. J. Heuvel |
title_short | Timing Neutron Stars |
title_sort | timing neutron stars |
topic | Physics Astrophysics and Astroparticles Statistics for Engineering, Physics, Computer Science, Chemistry and Earth Sciences |
topic_facet | Physics Astrophysics and Astroparticles Statistics for Engineering, Physics, Computer Science, Chemistry and Earth Sciences |
url | https://doi.org/10.1007/978-94-009-2273-0 |
work_keys_str_mv | AT ogelmanh timingneutronstars AT heuvelepj timingneutronstars AT ogelmanh proceedingsofthenatoadvancedstudyinstitutecesmeizmirturkey415april1988 AT heuvelepj proceedingsofthenatoadvancedstudyinstitutecesmeizmirturkey415april1988 |