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The Galactic and Extragalactic Background Radiation: Proceedings of the 139th Symposium of the International Astronomical Union Held in Heidelberg, ... (International Astronomical Union Symposia) - Tapa blanda
Sinopsis
The galactic and extragalactic background radiation components are of major importance in astrophysical studies of a variety of problems related to galactic structure, interstellar matter, the distribution and evolution of galaxies and intergalactic matter, and cosmology. The back ground radiation is a unique source of information in cases where the source is of a truly diffuse nature, as with scattering and emission by interstellar dust and gas, or where the discrete emission sources are so faint (e. g. , very distant galaxies) that they can be observed only by their integrated emission. The galactic and extragalactic background must be discussed together because they are observationally entangled and their proper separation requires a knowledge of both components. The above points are equally valid for the entire electromag netic spectrum, from gamma rays to long radio waves. Thus, the study of the galactic and extragalactic background radiation is interdisciplinary in its character, and a multi wavelength approach would appear to be dictated by the nature of the topic. The proper separation of the galactic and extragalactic background components requires a knowledge of both. In addition, the foreground components, i. e. , zodiacal light, airglow, and atmospheric scattered light, must be treated carefully.
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Reseña del editor
The galactic and extragalactic background radiation components are of major importance in astrophysical studies of a variety of problems related to galactic structure, interstellar matter, the distribution and evolution of galaxies and intergalactic matter, and cosmology. The back ground radiation is a unique source of information in cases where the source is of a truly diffuse nature, as with scattering and emission by interstellar dust and gas, or where the discrete emission sources are so faint (e. g. , very distant galaxies) that they can be observed only by their integrated emission. The galactic and extragalactic background must be discussed together because they are observationally entangled and their proper separation requires a knowledge of both components. The above points are equally valid for the entire electromag netic spectrum, from gamma rays to long radio waves. Thus, the study of the galactic and extragalactic background radiation is interdisciplinary in its character, and a multi wavelength approach would appear to be dictated by the nature of the topic. The proper separation of the galactic and extragalactic background components requires a knowledge of both. In addition, the foreground components, i. e. , zodiacal light, airglow, and atmospheric scattered light, must be treated carefully.
Reseña del editor
Proceedings of the 139th Symposium of the International Astronomical Union on The Galactic and Extragalactic Background Radiation, held in Heidelberg, FRG, June 12-16, 1989
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The Galactic and Extragalactic Background Radiation
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Springer Netherlands, 1990
ISBN 10: 0792308425
ISBN 13: 9780792308423
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Kartoniert / Broschiert. Condición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Proceedings of the 139th Symposium of the International Astronomical Union on `The Galactic and Extragalactic Background Radiation, held in Heidelberg, FRG, June 12-16, 1989 The galactic and extragalactic background radiation components are of maj. Nº de ref. del artículo: 5966033
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The Galactic and Extragalactic Background Radiation: Proceedings of the 139th Symposium of the International Astronomical Union Held in Heidelberg, ... Astronomical Union Symposia, 139)
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The Galactic and Extragalactic Background Radiation : Proceedings of the 139th Symposium of the International Astronomical Union Held in Heidelberg, F.R.G., June 12¿16, 1989
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Springer Netherlands, 1990
ISBN 10: 0792308425
ISBN 13: 9780792308423
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Taschenbuch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - The galactic and extragalactic background radiation components are of major importance in astrophysical studies of a variety of problems related to galactic structure, interstellar matter, the distribution and evolution of galaxies and intergalactic matter, and cosmology. The back ground radiation is a unique source of information in cases where the source is of a truly diffuse nature, as with scattering and emission by interstellar dust and gas, or where the discrete emission sources are so faint (e. g. , very distant galaxies) that they can be observed only by their integrated emission. The galactic and extragalactic background must be discussed together because they are observationally entangled and their proper separation requires a knowledge of both components. The above points are equally valid for the entire electromag netic spectrum, from gamma rays to long radio waves. Thus, the study of the galactic and extragalactic background radiation is interdisciplinary in its character, and a multi wavelength approach would appear to be dictated by the nature of the topic. The proper separation of the galactic and extragalactic background components requires a knowledge of both. In addition, the foreground components, i. e. , zodiacal light, airglow, and atmospheric scattered light, must be treated carefully. Nº de ref. del artículo: 9780792308423
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Galactic and Extragalactic Background Radiation : Proceedings of the 139th Symposium of the International Astronomical Union Held in Heidelberg, F.r.g., June 12?16, 1989
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Galactic and Extragalactic Background Radiation : Proceedings of the 139th Symposium of the International Astronomical Union Held in Heidelberg, F.r.g., June 12?16, 1989
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The Galactic and Extragalactic Background Radiation
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Springer Netherlands, Springer Netherlands Aug 1990, 1990
ISBN 10: 0792308425
ISBN 13: 9780792308423
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Taschenbuch. Condición: Neu. This item is printed on demand - Print on Demand Titel. Neuware -The galactic and extragalactic background radiation components are of major importance in astrophysical studies of a variety of problems related to galactic structure, interstellar matter, the distribution and evolution of galaxies and intergalactic matter, and cosmology. The back ground radiation is a unique source of information in cases where the source is of a truly diffuse nature, as with scattering and emission by interstellar dust and gas, or where the discrete emission sources are so faint (e. g. , very distant galaxies) that they can be observed only by their integrated emission. The galactic and extragalactic background must be discussed together because they are observationally entangled and their proper separation requires a knowledge of both components. The above points are equally valid for the entire electromag netic spectrum, from gamma rays to long radio waves. Thus, the study of the galactic and extragalactic background radiation is interdisciplinary in its character, and a multi wavelength approach would appear to be dictated by the nature of the topic. The proper separation of the galactic and extragalactic background components requires a knowledge of both. In addition, the foreground components, i. e. , zodiacal light, airglow, and atmospheric scattered light, must be treated carefully.Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 532 pp. Englisch. Nº de ref. del artículo: 9780792308423
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Galactic and Extragalactic Background Radiation : Proceedings of the 139th Symposium of the International Astronomical Union Held in Heidelberg, F.r.g., June 12?16, 1989
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Galactic and Extragalactic Background Radiation : Proceedings of the 139th Symposium of the International Astronomical Union Held in Heidelberg, F.r.g., June 12?16, 1989
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The Galactic and Extragalactic Background Radiation: Proceedings of the 139th Symposium of the International Astronomical Union Held in Heidelberg, F.R.G., June 12-16, 1989
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The Galactic and Extragalactic Background Radiation
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Condición: New. pp. 532. Nº de ref. del artículo: 26540662
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