L crivellari (37 risultati)
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Da: Antiquariat Thomas Haker GmbH & Co. KG, Berlin, GermaniaAntiquariat Thomas Haker GmbH & Co. KG
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EUR 7,92
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Condizione: Gut. 461 S. With figures. Guter Zustand/ Good Sprache: Englisch Gewicht in Gramm: 811 Hardcover/ Pappband fest gebunden.
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Da: Better World Books: West, Reno, NV, U.S.A.Better World Books: West
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EUR 71,38
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Condizione: Very Good. 1985th Edition. Former library copy. Pages intact with possible writing/highlighting. Binding strong with minor wear. Dust jackets/supplements may not be included. Includes library markings. Stock photo provided. Product includes identifying sticker. Better World Books: Buy Books. Do Good.
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Da: Ria Christie Collections, Uxbridge, Regno UnitoRia Christie Collections
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EUR 60,62
EUR 13,88 spedizioneSpedito da Regno Unito a U.S.A.Quantità: Più di 20 disponibili
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Da: Chiron Media, Wallingford, , Regno UnitoChiron Media
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EUR 57,25
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PF. Condizione: New.
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Da: Books Puddle, New York, NY, U.S.A.Books Puddle
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EUR 81,47
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Condizione: New. pp. 468 Index.
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Da: Revaluation Books, Exeter, , Regno UnitoRevaluation Books
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EUR 82,01
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Paperback. Condizione: Brand New. 468 pages. 9.25x6.10x1.06 inches. In Stock.
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Da: preigu, Osnabrück, Germaniapreigu
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EUR 50,25
EUR 70,00 spedizioneSpedito da Germania a U.S.A.Quantità: 5 disponibili
Taschenbuch. Condizione: Neu. Progress in Stellar Spectral Line Formation Theory | J. E. Beckman (u. a.) | Taschenbuch | 464 S. | Englisch | 2011 | Springer | EAN 9789401088701 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: prei…gu.
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Da: AHA-BUCH GmbH, Einbeck, GermaniaAHA-BUCH GmbH
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EUR 59,97
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Taschenbuch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - Spectral line formation theory is at the heart of astrophysical diagnostic. Our knowledge of abundances, in both stellar and interstellar contexts, comes almost enti rely from line analysis, as does a major fraction of our ability to model stellar… atmospheres. As new facets of the universe become observable so the techniques of high reso lution spectroscopy are brought to bear, with great reward. Improved instruments, such as echelle spectrographs, employ ing detectors of high quantum efficiency, have revolutioned our ability to observe high quality line profiles, although until now this ability has been confined to the brightest stars. Fabry-Perot interferometers and their modern deriva tives are bringing new ranges of resolving power to studies of atomic and ionic interstellar lines, and of course radio techniques imply exceedingly high resolution for the cool interstellar medium of molecules and radicals. Telescopes in space are extending the spectral range of these types of observations. Already the Copernicus and IUE high resolution spectrographs have given us a tantalizing glimmer of what it will be like to obtain ultraviolet spectra with resolution and signal to noise ratio approaching those obtainable on the ground. Fairly soon Space Telescope will be producing high resolution spectroscopic data of unparal leled quali ty and distance range. As often happens in astro physics the challenge is now coming from the observers to the theorists to provide interpretational tools which are adequate to the state of the data.
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Da: Doss-Haus Books, Redondo Beach, CA, U.S.A.Doss-Haus Books
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EUR 166,84
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Hardcover. Condizione: Very Good. No Jacket. Hardcover 1985 edition. Ex-library book with stamps and labels attached. Binding firm. Pages unmarked and clean. Covers and text in very good condition. Series: NATO ASI series. Series C: Mathematical and Physical Sciences ;Vol. 152. [xvi, 448 p. : ill. ; 25 cm].
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Da: GreatBookPricesUK, Woodford Green, Regno UnitoGreatBookPricesUK
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EUR 216,81
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Condizione: New.
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Da: Ria Christie Collections, Uxbridge, Regno UnitoRia Christie Collections
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EUR 225,59
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Condizione: New. In.
- Rilegato
Da: Ria Christie Collections, Uxbridge, Regno UnitoRia Christie Collections
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EUR 225,59
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Da: GreatBookPrices, Columbia, MD, U.S.A.GreatBookPrices
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EUR 239,16
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Condizione: New.
Altre immagini- Brossura
Da: preigu, Osnabrück, Germaniapreigu
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EUR 186,70
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Taschenbuch. Condizione: Neu. Stellar Atmospheres: Beyond Classical Models | L. Crivellari (u. a.) | Taschenbuch | xiv | Englisch | 2012 | Springer | EAN 9789401055741 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.
- Rilegato
Da: Books Puddle, New York, NY, U.S.A.Books Puddle
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EUR 279,05
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Condizione: New. pp. 480.
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Da: AHA-BUCH GmbH, Einbeck, GermaniaAHA-BUCH GmbH
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EUR 223,11
EUR 63,58 spedizioneSpedito da Germania a U.S.A.Quantità: 1 disponibili
Taschenbuch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - The theory of stellar atmospheres is one of the most important branches of modern astrophysics. It is first of all a major tool for understanding all aspects of stars. As the physical properties of their outer layers can now be found with high pre…cision, firm conclusions can be drawn about the internal structure and evolution of stars. Moreover, improvements in our knowledge of the chemical composition of stars is shedding new light on the chemical evolution of galaxies and of the Universe as a whole. Because the outer layers of stars are among the best-understood astrophysical objects, the theory of stellar atmospheres plays an important role in the study of many other types of objects. These include planetary nebulae, H II regions, interstellar matter, and objects of interest in high-energy astrophysics, such as accretion disks (close binaries, dwarf novae, cataclysmic variables, quasars, active galactic nuclei), pulsar magnetospheres, and Seyfert galaxies. Finally, as stars provide a laboratory in which plasmas can be studied under more extreme conditions than on earth, the study of stellar atmospheres has strong connections with modern physics. Astronomical observations provided a vital stimulus in the early stages of quantum theory and atomic physics; even today topics such as low-temperature dielectronic recombination develop hand in hand with the interpretation of stellar and nebular spectra. Early work on MHD was similiarly motivated. Many such connections remain to be explored.
- Rilegato
Da: AHA-BUCH GmbH, Einbeck, GermaniaAHA-BUCH GmbH
Contatta il venditoreVenditore con 5 stelleCondizione: Nuovo
EUR 223,11
EUR 64,41 spedizioneSpedito da Germania a U.S.A.Quantità: 1 disponibili
Buch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - The theory of stellar atmospheres is one of the most important branches of modern astrophysics. It is first of all a major tool for understanding all aspects of stars. As the physical properties of their outer layers can now be found with high precision,… firm conclusions can be drawn about the internal structure and evolution of stars. Moreover, improvements in our knowledge of the chemical composition of stars is shedding new light on the chemical evolution of galaxies and of the Universe as a whole. Because the outer layers of stars are among the best-understood astrophysical objects, the theory of stellar atmospheres plays an important role in the study of many other types of objects. These include planetary nebulae, H II regions, interstellar matter, and objects of interest in high-energy astrophysics, such as accretion disks (close binaries, dwarf novae, cataclysmic variables, quasars, active galactic nuclei), pulsar magnetospheres, and Seyfert galaxies. Finally, as stars provide a laboratory in which plasmas can be studied under more extreme conditions than on earth, the study of stellar atmospheres has strong connections with modern physics. Astronomical observations provided a vital stimulus in the early stages of quantum theory and atomic physics; even today topics such as low-temperature dielectronic recombination develop hand in hand with the interpretation of stellar and nebular spectra. Early work on MHD was similiarly motivated. Many such connections remain to be explored.
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Da: GreatBookPricesUK, Woodford Green, Regno UnitoGreatBookPricesUK
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EUR 311,46
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Condizione: As New. Unread book in perfect condition.
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Da: Mispah books, Redhill, SURRE, Regno UnitoMispah books
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EUR 301,92
EUR 28,97 spedizioneSpedito da Regno Unito a U.S.A.Quantità: 1 disponibili
Paperback. Condizione: Like New. Like New. book.
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Da: GreatBookPrices, Columbia, MD, U.S.A.GreatBookPrices
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EUR 338,44
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Condizione: As New. Unread book in perfect condition.
Editore: Tipografia Editrice Esca, Vicenza 2006
Da: Studio Bibliografico Malombra, Vicenza, VI, ItaliaStudio Bibliografico Malombra
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EUR 9,00
EUR 42,00 spedizioneSpedito da Italia a U.S.A.Quantità: 1 disponibili
113 p., qualche ill. in nero n.t.; 24 cm. Bross. edit. Leggerissime tracce di polvere in copertina, molto buono.
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- Print on Demand
Da: Brook Bookstore On Demand, Napoli, NA, ItaliaBrook Bookstore On Demand
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EUR 46,22
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Condizione: new. Questo è un articolo print on demand.
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Da: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, , GermaniaBuchWeltWeit Ludwig Meier e.K.
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EUR 53,49
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Taschenbuch. Condizione: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Spectral line formation theory is at the heart of astrophysical diagnostic. Our knowledge of abundances, in both stellar and interstellar contexts, comes almost enti rely from line analysis, as does a major fraction of our ability…to model stellar atmospheres. As new facets of the universe become observable so the techniques of high reso lution spectroscopy are brought to bear, with great reward. Improved instruments, such as echelle spectrographs, employ ing detectors of high quantum efficiency, have revolutioned our ability to observe high quality line profiles, although until now this ability has been confined to the brightest stars. Fabry-Perot interferometers and their modern deriva tives are bringing new ranges of resolving power to studies of atomic and ionic interstellar lines, and of course radio techniques imply exceedingly high resolution for the cool interstellar medium of molecules and radicals. Telescopes in space are extending the spectral range of these types of observations. Already the Copernicus and IUE high resolution spectrographs have given us a tantalizing glimmer of what it will be like to obtain ultraviolet spectra with resolution and signal to noise ratio approaching those obtainable on the ground. Fairly soon Space Telescope will be producing high resolution spectroscopic data of unparal leled quali ty and distance range. As often happens in astro physics the challenge is now coming from the observers to the theorists to provide interpretational tools which are adequate to the state of the data. 468 pp. Englisch.
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- Print on Demand
Da: Majestic Books, Hounslow, , Regno UnitoMajestic Books
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EUR 81,07
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Condizione: New. Print on Demand pp. 468 Figures, 49:B&W 6.14 x 9.21 in or 234 x 156 mm (Royal 8vo) Perfect Bound on White w/Gloss Lam.
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- Print on Demand
Da: Biblios, frankfurt am main, HESSE, GermaniaBiblios
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EUR 80,46
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Condizione: New. PRINT ON DEMAND pp. 468.
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Da: moluna, Greven, , Germaniamoluna
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EUR 48,37
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Condizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Proceedings of the NATO Advanced Research Workshop, Grignano-Miramare, Trieste, Italy, September 4-7, 1984 Spectral line formation theory is at the heart of astrophysical diagnostic. Our knowledge of abundances, in b…oth stellar and interstellar con.
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Da: buchversandmimpf2000, Emtmannsberg, BAYE, Germaniabuchversandmimpf2000
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Taschenbuch. Condizione: Neu. This item is printed on demand - Print on Demand Titel. Neuware -Spectral line formation theory is at the heart of astrophysical diagnostic. Our knowledge of abundances, in both stellar and interstellar contexts, comes almost enti rely from line analysis, as does a major fraction of our ability to m…odel stellar atmospheres. As new facets of the universe become observable so the techniques of high reso lution spectroscopy are brought to bear, with great reward. Improved instruments, such as echelle spectrographs, employ ing detectors of high quantum efficiency, have revolutioned our ability to observe high quality line profiles, although until now this ability has been confined to the brightest stars. Fabry-Perot interferometers and their modern deriva tives are bringing new ranges of resolving power to studies of atomic and ionic interstellar lines, and of course radio techniques imply exceedingly high resolution for the cool interstellar medium of molecules and radicals. Telescopes in space are extending the spectral range of these types of observations. Already the Copernicus and IUE high resolution spectrographs have given us a tantalizing glimmer of what it will be like to obtain ultraviolet spectra with resolution and signal to noise ratio approaching those obtainable on the ground. Fairly soon Space Telescope will be producing high resolution spectroscopic data of unparal leled quali ty and distance range. As often happens in astro physics the challenge is now coming from the observers to the theorists to provide interpretational tools which are adequate to the state of the data.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 468 pp. Englisch.
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Da: Brook Bookstore On Demand, Napoli, NA, ItaliaBrook Bookstore On Demand
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Condizione: new. Questo è un articolo print on demand.
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Da: moluna, Greven, , Germaniamoluna
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EUR 180,07
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Condizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Proceedings of the NATO Advanced Research Workshop, Trieste, Italy, September 3-7, 1990 The theory of stellar atmospheres is one of the most important branches of modern astrophysics. It is first of all a major tool…for understanding all aspects of sta.
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- Print on Demand
Da: moluna, Greven, , Germaniamoluna
Contatta il venditoreVenditore con 5 stelleCondizione: Nuovo
EUR 180,07
EUR 48,99 spedizioneSpedito da Germania a U.S.A.Quantità: Più di 20 disponibili
Gebunden. Condizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Proceedings of the NATO Advanced Research Workshop, Trieste, Italy, September 3-7, 1990 The theory of stellar atmospheres is one of the most important branches of modern astrophysics. It is first of all a m…ajor tool for understanding all aspects of sta.
