2010, ISBN: 3642067778

[EAN: 9783642067778], Libro nuovo, [SC: 14.99], [PU: Springer Berlin Heidelberg], EXTRAGALACTICASTRONOMY; EXTRASOLARPLANETS; COSMOLOGY; ASTRONOMY; ASTROPHYSICS; GALACTICHALOS; GALAXYCLUST… Mehr…

[EAN: 9783642067778], Libro nuovo, [SC: 14.99], [PU: Springer Berlin Heidelberg], EXTRAGALACTICASTRONOMY; EXTRASOLARPLANETS; COSMOLOGY; ASTRONOMY; ASTROPHYSICS; GALACTICHALOS; GALAXYCLUSTERS; GRAVITATIONALLENSING; GRAVITY; MICROLENSING, Druck auf Anfrage Neuware - Printed after ordering - The observation, in 1919 by A.S. Eddington and collaborators, of the gra- tational de ection of light by the Sun proved one of the many predictions of Einstein's Theory of General Relativity: The Sun was the rst example of a gravitational lens. In 1936, Albert Einstein published an article in which he suggested - ing stars as gravitational lenses. A year later, Fritz Zwicky pointed out that galaxies would act as lenses much more likely than stars, and also gave a list of possible applications, as a means to determine the dark matter content of galaxies and clusters of galaxies. It was only in 1979 that the rst example of an extragalactic gravitational lens was provided by the observation of the distant quasar QSO 0957+0561, by D. Walsh, R.F. Carswell, and R.J. Weymann. A few years later, the rst lens showing images in the form of arcs was detected. The theory, observations, and applications of gravitational lensing cons- tute one of the most rapidly growing branches of astrophysics. The gravi- tional de ection of light generated by mass concentrations along a light path producesmagni cation,multiplicity,anddistortionofimages,anddelaysp- ton propagation from one line of sight relative to another. The huge amount of scienti c work produced over the last decade on gravitational lensing has clearly revealed its already substantial and wide impact, and its potential for future astrophysical applications. 572 pp. Englisch, Books<

2010, ISBN: 3642067778

[EAN: 9783642067778], Neubuch, [SC: 0.0], [PU: Springer Berlin Heidelberg], EXTRAGALACTICASTRONOMY; EXTRASOLARPLANETS; COSMOLOGY; ASTRONOMY; ASTROPHYSICS; GALACTICHALOS; GALAXYCLUSTERS; G… Mehr…

[EAN: 9783642067778], Neubuch, [SC: 0.0], [PU: Springer Berlin Heidelberg], EXTRAGALACTICASTRONOMY; EXTRASOLARPLANETS; COSMOLOGY; ASTRONOMY; ASTROPHYSICS; GALACTICHALOS; GALAXYCLUSTERS; GRAVITATIONALLENSING; GRAVITY; MICROLENSING, Druck auf Anfrage Neuware - Printed after ordering - The observation, in 1919 by A.S. Eddington and collaborators, of the gra- tational de ection of light by the Sun proved one of the many predictions of Einstein's Theory of General Relativity: The Sun was the rst example of a gravitational lens. In 1936, Albert Einstein published an article in which he suggested - ing stars as gravitational lenses. A year later, Fritz Zwicky pointed out that galaxies would act as lenses much more likely than stars, and also gave a list of possible applications, as a means to determine the dark matter content of galaxies and clusters of galaxies. It was only in 1979 that the rst example of an extragalactic gravitational lens was provided by the observation of the distant quasar QSO 0957+0561, by D. Walsh, R.F. Carswell, and R.J. Weymann. A few years later, the rst lens showing images in the form of arcs was detected. The theory, observations, and applications of gravitational lensing cons- tute one of the most rapidly growing branches of astrophysics. The gravi- tional de ection of light generated by mass concentrations along a light path producesmagni cation,multiplicity,anddistortionofimages,anddelaysp- ton propagation from one line of sight relative to another. The huge amount of scienti c work produced over the last decade on gravitational lensing has clearly revealed its already substantial and wide impact, and its potential for future astrophysical applications., Books<

2013, ISBN: 9783642067778

[ED: Taschenbuch], [PU: Springer Berlin Heidelberg], Neuware - The observation, in 1919 by A.S. Eddington and collaborators, of the gra- tational de ection of light by the Sun proved one … Mehr…

[ED: Taschenbuch], [PU: Springer Berlin Heidelberg], Neuware - The observation, in 1919 by A.S. Eddington and collaborators, of the gra- tational de ection of light by the Sun proved one of the many predictions of Einstein's Theory of General Relativity: The Sun was the rst example of a gravitational lens. In 1936, Albert Einstein published an article in which he suggested - ing stars as gravitational lenses. A year later, Fritz Zwicky pointed out that galaxies would act as lenses much more likely than stars, and also gave a list of possible applications, as a means to determine the dark matter content of galaxies and clusters of galaxies. It was only in 1979 that the rst example of an extragalactic gravitational lens was provided by the observation of the distant quasar QSO 0957+0561, by D. Walsh, R.F. Carswell, and R.J. Weymann. A few years later, the rst lens showing images in the form of arcs was detected. The theory, observations, and applications of gravitational lensing cons- tute one of the most rapidly growing branches of astrophysics. The gravi- tional de ection of light generated by mass concentrations along a light path producesmagni cation,multiplicity,anddistortionofimages,anddelaysp- ton propagation from one line of sight relative to another. The huge amount of scienti c work produced over the last decade on gravitational lensing has clearly revealed its already substantial and wide impact, and its potential for future astrophysical applications.- Besorgungstitel - vorauss. Lieferzeit 3-5 Tage., DE, [SC: 0.00], Neuware, gewerbliches Angebot, 235x155x30 mm, 572, [GW: 855g], Banküberweisung, Offene Rechnung, Kreditkarte, PayPal, Offene Rechnung (Vorkasse vorbehalten), Internationaler Versand<

2010, ISBN: 9783642067778

[ED: Softcover], [PU: Springer / Springer Berlin Heidelberg / Springer, Berlin], The observation, in 1919 by A.S. Eddington and collaborators, of the gra- tational de?ection of light by t… Mehr…

[ED: Softcover], [PU: Springer / Springer Berlin Heidelberg / Springer, Berlin], The observation, in 1919 by A.S. Eddington and collaborators, of the gra- tational de?ection of light by the Sun proved one of the many predictions of Einstein's Theory of General Relativity: The Sun was the ?rst example of a gravitational lens. In 1936, Albert Einstein published an article in which he suggested - ing stars as gravitational lenses. A year later, Fritz Zwicky pointed out that galaxies would act as lenses much more likely than stars, and also gave a list of possible applications, as a means to determine the dark matter content of galaxies and clusters of galaxies. It was only in 1979 that the ?rst example of an extragalactic gravitational lens was provided by the observation of the distant quasar QSO 0957+0561, by D. Walsh, R.F. Carswell, and R.J. Weymann. A few years later, the ?rst lens showing images in the form of arcs was detected. The theory, observations, and applications of gravitational lensing cons- tute one of the most rapidly growing branches of astrophysics. The gravi- tional de?ection of light generated by mass concentrations along a light path producesmagni?cation,multiplicity,anddistortionofimages,anddelaysp- ton propagation from one line of sight relative to another. The huge amount of scienti?c work produced over the last decade on gravitational lensing has clearly revealed its already substantial and wide impact, and its potential for future astrophysical applications. 2010. xvi, 552 S. XVI, 552 p. 235 mm Versandfertig in 6-10 Tagen, DE, [SC: 0.00], Neuware, gewerbliches Angebot, Offene Rechnung (Vorkasse vorbehalten)<

ISBN: 9783642067778

Paperback, [PU: Springer-Verlag Berlin and Heidelberg GmbH & Co. KG], Swiss Society for Astrophysics and Astronomy, Astrophysics