Meylan georges (55 resultados)

Soft cover. Condición: Fine. Fine contents and binding. 2003, English text. 67 pp. with numerous color photographs of watches and time pieces.

Hardcover. Condición: Very good. Saas-Fee Advanced Course 33. Octavo: 552 p. with 196 illustrations, including 36 in color. Original glossy boards; issued without a dust jacket. The top corner of the rear board is bumped; else a crisp and clean copy. Better than very good.

Hardcover. Condición: Like New. First Edition. Firm, square and tight with sturdy hinges, just showing a few minor rubs and some mild cosmetic wear. Hence a non-text page is stamped 'damaged'. Despite such this book is in nearly new condition. Thus the contents are crisp, fresh and clean. Offered for sale at a very sensible price.…

Hardcover. Condición: Very Good. No Jacket. Full colour Catalogue of fine Wristwatches. 117 p. pages. 10 1/2" Tall. Small dent on front cover and a few on the back. Pages in fine condition. No inscriptions.

Condición: As New. Unread book in perfect condition.

Condición: New.

Condición: New. pp. xxiii + 471.

Paperback. Condición: Brand New. reprint edition. 494 pages. 9.25x6.10x1.20 inches. In Stock.

Taschenbuch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - The controversial question of whether the majority of the narrow absorption lines observed in QSO spectra represent cosmological intervening systems or ejecta from the QSO themselves is settled. QSO absorption line spectroscopy, initially a mere technique, has matured into an essential extragalactic research tool for understanding the content of the Universe at redshifts between 0 and 4, and beyond. The only previous important meeting devoted to 'QSO Absorption Lines' was held in May 1987 at the Space Telescope Science Institute in Baltimore, Maryland, U.S.A. Since that time, nearly a decade ago, research has been ex tremely active in this now well-established field of astrophysics. Theoretical stud ies and simulations have taken advantage of the constant progress in computer technology, and during these last few years, the observational results have bene fited largely from the new facillities offered by the Hubble Space Telescope in the UV wavelength range and the Keck Telescope for high-resolution spectroscopy.…

Condición: New.

Paperback. Condición: new. Paperback. The theory, observations, and applications of gravitational lensing constitute one of the most rapidly growing branches of astrophysics. The gravitational deflection of light generated by mass concentrations along a light path produces magnification, multiplicity, and distortion of images and delays photon propagation from one line of sight relative to another. The huge amount of scientific 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. The up-to-date contributions in this book are based on the lecture notes of the 33rd Saas--Fee Advanced Course of the Swiss Society of Astronomy and Astrophysics, entitled Gravitational Lensing: Strong, Weak, and Micro. The book comprises four complementary parts, written by leading experts in the field, constituting a genuine textbook about gravitational lensing. Students and researchers alike will benefit from this comprehensive presentation of the astrophysical and astronomical aspects of gravitational lensing. 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. Shipping may be from multiple locations in the US or from the UK, depending on stock availability. …

Condición: As New. Unread book in perfect condition.

Condición: New.

Condición: New.

Condición: New.

Opbd, geb., Großformat, 101 Seiten, obere Ecke des Covers etwas gestaucht, ans. frisches Ex. (gern Foto).

Condición: New.

Condición: New.

Condición: New.

Gebunden. Condición: New.

Condición: As New. Unread book in perfect condition.

hardcover. Condición: New. In shrink wrap. Looks like an interesting title.

Hardback. Condición: New. 2006 ed. 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.…

Taschenbuch. Condición: Neu. 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.…

Taschenbuch. Condición: Neu. Gravitational Lensing: Strong, Weak and Micro | Saas-Fee Advanced Course 33 | Peter Schneider (u. a.) | Taschenbuch | Saas-Fee Advanced Course | xvi | Englisch | 2010 | Springer | EAN 9783642067778 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu. …

Buch. Condición: Neu. 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.…

Hardcover. Condición: Brand New. 1st edition. 552 pages. 9.25x6.25x0.75 inches. In Stock.

Paperback. Condición: Brand New. reprint edition. 568 pages. 11.65x8.27x1.26 inches. In Stock.

Condición: New. pp. xvi + 552.

Hardcover. Condición: Like New. LIKE NEW. SHIPS FROM MULTIPLE LOCATIONS. book.