Stellar Atmospheres Beyond Classical (18 results)

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    • Language: English

      Published by Kluwer Academic Publishers Dordrecht, 1982

      0792313437 / 9780792313434

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      Seller: Antiquariat Thomas Haker GmbH & Co. KG, Berlin, GermanyAntiquariat Thomas Haker GmbH & Co. KG

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      Condition: Gut. 461 S. With figures. Guter Zustand/ Good Sprache: Englisch Gewicht in Gramm: 811 Hardcover/ Pappband fest gebunden.

    • Language: English

      Published by Springer, 2012

      9401055742 / 9789401055741

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    • Language: English

      Published by Springer, 2012

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      Seller: Ria Christie Collections, Uxbridge, United KingdomRia Christie Collections

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      Condition: New. In English.

    • Language: English

      Published by Springer, 1991

      0792313437 / 9780792313434

      • Hardcover

      Seller: Ria Christie Collections, Uxbridge, United KingdomRia Christie Collections

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      Condition: New. In English.

    • Language: English

      Published by Springer, 2012

      9401055742 / 9789401055741

      • Softcover

      Seller: GreatBookPrices, Columbia, MD, U.S.A.GreatBookPrices

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    • Language: English

      Published by Springer, Springer, 2012

      9401055742 / 9789401055741

      • Softcover

      Seller: AHA-BUCH GmbH, Einbeck, GermanyAHA-BUCH GmbH

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      Taschenbuch. Condition: 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.

    • Language: English

      Published by Springer, 1991

      0792313437 / 9780792313434

      • Hardcover

      Seller: AHA-BUCH GmbH, Einbeck, GermanyAHA-BUCH GmbH

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      Buch. Condition: 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.

    • Language: English

      Published by Springer, 2012

      9401055742 / 9789401055741

      • Softcover

      Seller: GreatBookPricesUK, Woodford Green, United KingdomGreatBookPricesUK

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    • Language: English

      Published by Springer, 2012

      9401055742 / 9789401055741

      • Softcover

      Seller: Mispah books, Redhill, SURRE, United KingdomMispah books

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      Paperback. Condition: Like New. LIKE NEW. SHIPS FROM MULTIPLE LOCATIONS. book.

    • Language: English

      Published by Springer, 2012

      9401055742 / 9789401055741

      • Softcover

      Seller: GreatBookPrices, Columbia, MD, U.S.A.GreatBookPrices

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    • Language: English

      Published by Springer, 2012

      9401055742 / 9789401055741

      • Softcover
      • Print on Demand

      Seller: Brook Bookstore On Demand, Napoli, NA, ItalyBrook Bookstore On Demand

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      Condition: new. Questo è un articolo print on demand.

    • Language: English

      Published by Springer Netherlands, 1991

      0792313437 / 9780792313434

      • Hardcover
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      Seller: moluna, Greven, Germanymoluna

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      Gebunden. Condition: 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.

    • Language: English

      Published by Springer Netherlands, 2012

      9401055742 / 9789401055741

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      Seller: moluna, Greven, Germanymoluna

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      Condition: 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.

    • Language: English

      Published by Springer, Springer Netherlands Okt 2012, 2012

      9401055742 / 9789401055741

      • Softcover
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      Seller: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, GermanyBuchWeltWeit Ludwig Meier e.K.

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      Taschenbuch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -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. 476 pp. Englisch.

    • Language: English

      Published by Springer Netherlands Jul 1991, 1991

      0792313437 / 9780792313434

      • Hardcover
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      Seller: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, GermanyBuchWeltWeit Ludwig Meier e.K.

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      Buch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -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. 480 pp. Englisch.

    • Language: English

      Published by Springer Netherland, 1991

      0792313437 / 9780792313434

      • Hardcover
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      Seller: preigu, Osnabrück, Germanypreigu

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      Buch. Condition: Neu. Stellar Atmospheres: Beyond Classical Models | L. Crivellari (u. a.) | Buch | Einband - fest (Hardcover) | Englisch | 1991 | Springer Netherland | EAN 9780792313434 | Verantwortliche Person für die EU: Springer Netherlands, Haberstr. 7, 69126 Heidelberg, buchhandel-buch[at]springer[dot]com | Anbieter: preigu Print on Demand.

    • Language: English

      Published by Springer, Springer Okt 2012, 2012

      9401055742 / 9789401055741

      • Softcover
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      Seller: buchversandmimpf2000, Emtmannsberg, BAYE, Germanybuchversandmimpf2000

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      Taschenbuch. Condition: Neu. This item is printed on demand - Print on Demand Titel. Neuware -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.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 476 pp. Englisch.

    • Language: English

      Published by Springer Netherlands, Springer Netherlands Jul 1991, 1991

      0792313437 / 9780792313434

      • Hardcover
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      Seller: buchversandmimpf2000, Emtmannsberg, BAYE, Germanybuchversandmimpf2000

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      Buch. Condition: Neu. This item is printed on demand - Print on Demand Titel. Neuware -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.Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 480 pp. Englisch.