PSR B1829-10 (parfois abrégé PSR 1829-10 dans l'ancienne nomenclature) est un pulsar se situant à approximativement 30 000 années-lumière dans la constellation de l'Écu de Sobieski.

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dbpedia-owl:abstract
  • PSR B1829-10 (parfois abrégé PSR 1829-10 dans l'ancienne nomenclature) est un pulsar se situant à approximativement 30 000 années-lumière dans la constellation de l'Écu de Sobieski.
  • PSR B1829-10 (often shortened to PSR 1829-10) is a pulsar that is approximately 30,000 light-years away in the constellation of Scutum. This pulsar has been the target of interest, because of a mistaken identification of a planet around it. Andrew G. Lyne of the University of Manchester and Bailes claimed in July 1991 to have found "a planet orbiting the neutron star PSR1829-10" but in 1992 retracted. They had failed to correctly take into account the ellipticity of Earth's orbit, and had incorrectly concluded that a planet with an orbital period of half a year existed around the pulsar.
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  • 23 (xsd:integer)
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dbpedia-owl:wikiPageWikiLink
prop-fr:année
  • 1997 (xsd:integer)
prop-fr:auteur
  • Bailes et al.
  • Lin et al.
  • Lyne et al.
  • Podsiadlowski et al.
prop-fr:consultéLe
  • 2008-07-03 (xsd:date)
prop-fr:date
  • 1991-07-25 (xsd:date)
  • 1991-08-29 (xsd:date)
  • 1991-10-31 (xsd:date)
  • 1992-01-16 (xsd:date)
prop-fr:langue
  • en
  • Portuguese
prop-fr:nom
  • Dieguez
  • Krolik
prop-fr:prénom
  • Flávio
  • Julian H.
prop-fr:série
prop-fr:titre
  • A planet orbiting the neutron star PSR1829–10
  • No planet orbiting PS R1829–10
  • Terra à vista
  • The origin of the planet orbiting PSR1829 – 10
  • Formation of a planet orbiting pulsar 1829–10 from the debris of a supernova explosion
  • The Search for the Extrasolar Planets: A Brief History of the Search, the Findings and the Future Implications
  • Creation by stellar ablation of the low-mass companion to pulsar 1829–10
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dcterms:subject
rdfs:comment
  • PSR B1829-10 (parfois abrégé PSR 1829-10 dans l'ancienne nomenclature) est un pulsar se situant à approximativement 30 000 années-lumière dans la constellation de l'Écu de Sobieski.
  • PSR B1829-10 (often shortened to PSR 1829-10) is a pulsar that is approximately 30,000 light-years away in the constellation of Scutum. This pulsar has been the target of interest, because of a mistaken identification of a planet around it. Andrew G. Lyne of the University of Manchester and Bailes claimed in July 1991 to have found "a planet orbiting the neutron star PSR1829-10" but in 1992 retracted.
rdfs:label
  • PSR B1829-10
  • PSR B1829−10
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