Home > Binaire X Faible Masse: Grs 1915]105, Gx 339-4, Gro J1655-40, Rapid Burster, Scorpius X-1, Sagittarius X-4, Xte J1819-254, V404 Cygni(French)
Binaire X Faible Masse: Grs 1915]105, Gx 339-4, Gro J1655-40, Rapid Burster, Scorpius X-1, Sagittarius X-4, Xte J1819-254, V404 Cygni(French)

Binaire X Faible Masse: Grs 1915]105, Gx 339-4, Gro J1655-40, Rapid Burster, Scorpius X-1, Sagittarius X-4, Xte J1819-254, V404 Cygni(French)

          
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About the Book

Les achats comprennent une adhsion l'essai gratuite au club de livres de l'diteur, dans lequel vous pouvez choisir parmi plus d'un million d'ouvrages, sans frais. Le livre consiste d'articles Wikipedia sur: Grs 1915]105, Gx 339-4, Gro J1655-40, Rapid Burster, Scorpius X-1, Sagittarius X-4, Xte J1819-254, V404 Cygni, 1a 0620-00. Non illustr. Mises jour gratuites en ligne. Extrait: GRS 1915+105 (aussi appel V1487 Aquilae ou Nova Aquilae 1992) est un microquasar dans notre Galaxie situ dans la constellation de l'Aigle. Il contient un trou noir stellaire en orbite avec une toile ordinaire dont il arrache une partie de la masse. Il fut, en 1994, le premier objet galactique o des jets radio superluminiques furent observs et le premier astrophysique o le phnomne de jet supraluminique fut tabli avec certitude, les autres candidats existant tant plus loin, voluant plus lentement et tant de ce fait plus difficiles interprter. GRS 1915+105 fut dcouverte par le satellite artificiel franco-russe Granat le 15 aot 1992, lors d'une phase d'activit qui vit son mission en X avoir un surcrot important d'intensit. Ce phnomne lui valut galement une dsignation de nova, en l'occurrence Nova Aquilae 1992, mais cette dsignation est nettement moins commune que la dsignation Granat GRS 1915+105. La premire tentative d'association une contrepartie optique choua en 1993. La mme anne, GRS 1915+105 put tre observ en radio par le Very Large Array (VLA), qui montra galement une forte augmentation de luminosit, consquence du regain d'activit de 1992. Cette observation permit de dterminer avec grande prcision la localisation exacte de cet objet, puis sa contrepartie dans le domaine infrarouge. GRS 1915+105 est une binaire X faible masse, c'est--dire que son toile compagnon est une toile de la squence principale de faible masse, dont le type spectral est K/M III. Elle forme avec elle une orbite relativemen...http: //booksllc.net/?l=fr


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Product Details
  • ISBN-13: 9781159633332
  • Publisher: Books LLC
  • Publisher Imprint: Books LLC
  • Height: 152 mm
  • No of Pages: 40
  • Series Title: French
  • Sub Title: Grs 1915]105, Gx 339-4, Gro J1655-40, Rapid Burster, Scorpius X-1, Sagittarius X-4, Xte J1819-254, V404 Cygni
  • Width: 229 mm
  • ISBN-10: 1159633339
  • Publisher Date: 31 Jul 2010
  • Binding: Paperback
  • Language: French
  • Returnable: N
  • Spine Width: 2 mm
  • Weight: 73 gr


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Binaire X Faible Masse: Grs 1915]105, Gx 339-4, Gro J1655-40, Rapid Burster, Scorpius X-1, Sagittarius X-4, Xte J1819-254, V404 Cygni(French)
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Binaire X Faible Masse: Grs 1915]105, Gx 339-4, Gro J1655-40, Rapid Burster, Scorpius X-1, Sagittarius X-4, Xte J1819-254, V404 Cygni(French)
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Binaire X Faible Masse: Grs 1915]105, Gx 339-4, Gro J1655-40, Rapid Burster, Scorpius X-1, Sagittarius X-4, Xte J1819-254, V404 Cygni(French)

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