Sprache: Englisch
Verlag: Princeton University Press, 2014
ISBN 10: 0691163294 ISBN 13: 9780691163291
Anbieter: Better World Books, Mishawaka, IN, USA
Zustand: Very Good. 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.
Sprache: Englisch
Verlag: Kluwer Academic Publishers Dordrecht, 1982
ISBN 10: 0792313437 ISBN 13: 9780792313434
Anbieter: Antiquariat Thomas Haker GmbH & Co. KG, Berlin, Deutschland
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In den WarenkorbZustand: Gut. 461 S. With figures. Guter Zustand/ Good Sprache: Englisch Gewicht in Gramm: 811 Hardcover/ Pappband fest gebunden.
Sprache: Englisch
Verlag: Princeton University Press (edition ), 2014
ISBN 10: 0691163294 ISBN 13: 9780691163291
Anbieter: BooksRun, Philadelphia, PA, USA
Paperback. Zustand: Very Good. It's a well-cared-for item that has seen limited use. The item may show minor signs of wear. All the text is legible, with all pages included. It may have slight markings and/or highlighting.
Sprache: Englisch
Verlag: Princeton University Press (edition ), 2014
ISBN 10: 0691163294 ISBN 13: 9780691163291
Anbieter: BooksRun, Philadelphia, PA, USA
Paperback. Zustand: New. The item is brand new, never used or read. It's in perfect condition and may include supplements and/or access codes or come shrink-wrapped.
Sprache: Englisch
Verlag: Princeton University Press, Princeton, 2015
ISBN 10: 0691163286 ISBN 13: 9780691163284
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In den WarenkorbPaperback. Zustand: Very Good. Softback in very good condition. Light shelf and handling wear only, occasional very small dog-eared crease to bottom corners within text block, otherwise in 'as unread' condition. CN. Used.
Sprache: Englisch
Verlag: Princeton University Press, 2014
ISBN 10: 0691163294 ISBN 13: 9780691163291
Anbieter: PBShop.store US, Wood Dale, IL, USA
PAP. Zustand: New. New Book. Shipped from UK. Established seller since 2000.
Sprache: Englisch
Verlag: Cambridge University Press, 2012
ISBN 10: 1107019826 ISBN 13: 9781107019829
Anbieter: Ria Christie Collections, Uxbridge, Vereinigtes Königreich
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Sprache: Englisch
Verlag: San Francisco, Astronomical Society of the Pacific,, 2003
Anbieter: Buch & Cafe Antiquarius, Bonn, NRW, Deutschland
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Gr.-8°, original hardcover. 1. ed. With numerous images, XXV, 697 p. Rare copy. Shelfmark on spine, stamp on title, otherwise fine copy. Sprache: Englisch Gewicht in Gramm: 0.
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In den WarenkorbPaperback. Zustand: Brand New. 923 pages. 9.50x6.75x2.00 inches. In Stock.
Sprache: Englisch
Verlag: Princeton University Press, 2014
ISBN 10: 0691163294 ISBN 13: 9780691163291
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In den WarenkorbPAP. Zustand: New. New Book. Shipped from UK. Established seller since 2000.
Sprache: Englisch
Verlag: Princeton University Press, 2014
ISBN 10: 0691163294 ISBN 13: 9780691163291
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In den WarenkorbZustand: New. pp. 930.
Sprache: Englisch
Verlag: Princeton University Press, 2014
ISBN 10: 0691163294 ISBN 13: 9780691163291
Anbieter: Kennys Bookstore, Olney, MD, USA
Zustand: New. Series: Princeton Series in Astrophysics. Num Pages: 944 pages, 90 line illus. 17 tables. BIC Classification: PHVB; PNFS. Category: (P) Professional & Vocational; (U) Tertiary Education (US: College). Dimension: 157 x 235 x 53. Weight in Grams: 1568. . 2014. Paperback. . . . . Books ship from the US and Ireland.
Sprache: Englisch
Verlag: American Institute of Physics, 2009
ISBN 10: 073540710X ISBN 13: 9780735407107
Anbieter: Majestic Books, Hounslow, Vereinigtes Königreich
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In den WarenkorbZustand: New. pp. ix + 368 Illus.
Sprache: Englisch
Verlag: Cambridge University Press, 2012
ISBN 10: 1107019826 ISBN 13: 9781107019829
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In den WarenkorbHardcover. Zustand: Brand New. 568 pages. 10.00x7.00x1.25 inches. In Stock.
Sprache: Englisch
Verlag: Cambridge University Press, 2012
ISBN 10: 1107019826 ISBN 13: 9781107019829
Anbieter: AHA-BUCH GmbH, Einbeck, Deutschland
Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - In IAU Symposium 282, members of the exoplanet and binary star communities unite for the first time to discuss the state-of-the-art discovery, imaging, modeling and analysis tools used to study stars, brown dwarfs and exoplanets in multiple-object systems. They describe detection techniques using advanced telescopes and detectors, including the Kepler mission and the proposed Gaia and LSST projects. Imaging techniques discussed include adaptive optics, interferometry, polarimetry and tomography, while key modeling tools are covered in detail. Other topics include simulations of formation mechanisms in binary star systems, non-conservative evolution of binary stars, the formation and evolution of planets and a theory for the structure, atmospheres and evolution of giant exoplanets. The volume concludes with hydrodynamic simulations, models of planetary atmospheres and the habitability of exoplanets. These proceedings demonstrate how sophisticated modeling codes bridge the gap between theory and observations and increase our understanding of binary and multiple systems.
Sprache: Englisch
Verlag: Cambridge University Press, 2012
ISBN 10: 1107019826 ISBN 13: 9781107019829
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EUR 178,28
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In den WarenkorbZustand: New. In-depth summary and discussion of the state-of-the-art techniques used to study stars, brown dwarfs and exoplanets in multiple-object systems. Editor(s): Richards, Mercedes T.; Hubeny, Ivan. Series: Proceedings of the International Astronomical Union Symposia and Colloquia. Num Pages: 600 pages, 202 b/w illus. 36 tables. BIC Classification: PG. Category: (P) Professional & Vocational. Dimension: 252 x 181 x 29. Weight in Grams: 1184. . 2012. New. hardcover. . . . . Books ship from the US and Ireland.
Zustand: Sehr gut. Zustand: Sehr gut | Seiten: 368 | Sprache: Englisch | Produktart: Bücher | Keine Beschreibung verfügbar.
Anbieter: Ria Christie Collections, Uxbridge, Vereinigtes Königreich
EUR 225,54
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In den WarenkorbZustand: New. In.
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In den WarenkorbZustand: New. In.
Taschenbuch. Zustand: 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.
Taschenbuch. Zustand: 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.
Sprache: Englisch
Verlag: Springer Netherlands, Springer Netherlands, 1991
ISBN 10: 0792313437 ISBN 13: 9780792313434
Anbieter: AHA-BUCH GmbH, Einbeck, Deutschland
Buch. Zustand: 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.