Articles liés à Planets in Binary Star Systems
Planets in Binary Star Systems - Couverture souple
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Synopsis
In 1988, in an article on the analysis of the measurements of the variations in the radial velocities of a number of stars, Campbell, Walker, and Yang reported an - teresting phenomenon;the radial velocity variations of Cephei seemed to suggest the existence of a Jupiter-like planet around this star. This was a very exciting and, at the same time, very surprising discovery. It was exciting because if true, it would have marked the detection of the ?rst planet outside of our solar system. It was surprising because the planet-hosting star is the primary of a binary system with a separation less than 19 AU, a distance comparable to the planetary distances in our solar system. The moderatelyclose orbit of the stellar companionof Cephei raised questions about the reality of its planet. The skepticism over the interpretation of the results (which was primarily based on the idea that binary star systems with small sepa- tions would not be favorable places for planet formation) became so strong that in a subsequent paper in 1992, Walker and his colleagues suggested that the planet in the Cephei binary might not be real, and the variations in the radial velocity of this star might have been due to its chromospheric activities.
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Présentation de l'éditeur
The discovery of extrasolar planets has impacted on our understanding of planetary systems. This volume collates research into planets in binary and multistar systems and aims to familiarize readers with its associated theoretical and observational challenges.
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Planets in Binary Star Systems (eng)
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Planets in Binary Star Systems (Astrophysics and Space Science Library, 366)
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Planets in Binary Star Systems
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Springer Netherlands Sep 2012, 2012
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Taschenbuch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -In 1988, in an article on the analysis of the measurements of the variations in the radial velocities of a number of stars, Campbell, Walker, and Yang reported an - teresting phenomenon;the radial velocity variations of Cephei seemed to suggest the existence of a Jupiter-like planet around this star. This was a very exciting and, at the same time, very surprising discovery. It was exciting because if true, it would have marked the detection of the rst planet outside of our solar system. It was surprising because the planet-hosting star is the primary of a binary system with a separation less than 19 AU, a distance comparable to the planetary distances in our solar system. The moderatelyclose orbit of the stellar companionof Cephei raised questions about the reality of its planet. The skepticism over the interpretation of the results (which was primarily based on the idea that binary star systems with small sepa- tions would not be favorable places for planet formation) became so strong that in a subsequent paper in 1992, Walker and his colleagues suggested that the planet in the Cephei binary might not be real, and the variations in the radial velocity of this star might have been due to its chromospheric activities. 340 pp. Englisch. N° de réf. du vendeur 9789400732421
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Planets in Binary Star Systems
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Springer Netherlands, 2012
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ISBN 13 : 9789400732421
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Couverture souple
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Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. This volume presents the reader with the current state of the research on the detection and formation of planets in binary stars, written by teams of experts on these topics.In 1988, in an article on the analysis of the measurements of the variat. N° de réf. du vendeur 5826299
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Planets in Binary Star Systems
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Taschenbuch. Etat : Neu. Planets in Binary Star Systems | Nader Haghighipour | Taschenbuch | Astrophysics and Space Science Library | viii | Englisch | 2012 | Springer | EAN 9789400732421 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu. N° de réf. du vendeur 106297661
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Planets in Binary Star Systems
Edité par
Springer, Springer Sep 2012, 2012
ISBN 10 : 9400732422
ISBN 13 : 9789400732421
Neuf
Taschenbuch
Vendeur : buchversandmimpf2000, Emtmannsberg, BAYE, Allemagne
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Taschenbuch. Etat : Neu. This item is printed on demand - Print on Demand Titel. Neuware -In 1988, in an article on the analysis of the measurements of the variations in the radial velocities of a number of stars, Campbell, Walker, and Yang reported an - teresting phenomenon;the radial velocity variations of Cephei seemed to suggest the existence of a Jupiter-like planet around this star. This was a very exciting and, at the same time, very surprising discovery. It was exciting because if true, it would have marked the detection of the rst planet outside of our solar system. It was surprising because the planet-hosting star is the primary of a binary system with a separation less than 19 AU, a distance comparable to the planetary distances in our solar system. The moderatelyclose orbit of the stellar companionof Cephei raised questions about the reality of its planet. The skepticism over the interpretation of the results (which was primarily based on the idea that binary star systems with small sepa- tions would not be favorable places for planet formation) became so strong that in a subsequent paper in 1992, Walker and his colleagues suggested that the planet in the Cephei binary might not be real, and the variations in the radial velocity of this star might have been due to its chromospheric activities.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 340 pp. Englisch. N° de réf. du vendeur 9789400732421
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Planets in Binary Star Systems
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Taschenbuch. Etat : Neu. Druck auf Anfrage Neuware - Printed after ordering - In 1988, in an article on the analysis of the measurements of the variations in the radial velocities of a number of stars, Campbell, Walker, and Yang reported an - teresting phenomenon;the radial velocity variations of Cephei seemed to suggest the existence of a Jupiter-like planet around this star. This was a very exciting and, at the same time, very surprising discovery. It was exciting because if true, it would have marked the detection of the rst planet outside of our solar system. It was surprising because the planet-hosting star is the primary of a binary system with a separation less than 19 AU, a distance comparable to the planetary distances in our solar system. The moderatelyclose orbit of the stellar companionof Cephei raised questions about the reality of its planet. The skepticism over the interpretation of the results (which was primarily based on the idea that binary star systems with small sepa- tions would not be favorable places for planet formation) became so strong that in a subsequent paper in 1992, Walker and his colleagues suggested that the planet in the Cephei binary might not be real, and the variations in the radial velocity of this star might have been due to its chromospheric activities. N° de réf. du vendeur 9789400732421
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Planets in Binary Star Systems
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Paperback. Etat : Brand New. 2010 edition. 350 pages. 9.25x6.10x0.80 inches. In Stock. N° de réf. du vendeur x-9400732422
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Planets in Binary Star Systems (Astrophysics and Space Science Library (366))
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ISBN 10 : 9400732422
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