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Da: Librodifaccia, Alessandria, AL, Italia
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Hardcover. Condizione: VERY GOOD. Ex-lib, sound and square otherwise, very clean and sharp.
Editore: Talleres Graficos de Ind. Graf. Comuneros S.A., SPAGNA, 1988
ISBN 13: 2560731919746
Da: Biblioteca di Babele, Tarquinia, VT, Italia
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Aggiungi al carrelloCondizione: BUONO USATO. SPAGNOLO Coautore del volume Gustavo Adolfo Vittone. Legatura in cartonato illustrata con piccolo strappetto alla cerniera del piatto anteriore e lievi segni d'uso. Pagine ottimamente conservate, ben salde e con diverse carte geografiche fuori testo. Segnapagina in stoffa rosso. Numero Pagine 286.
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Editore: Edizioni Musicali Gamma, Genova, 1956
Da: Antica Libreria di Bugliarello Bruno S.A.S., San Gregorio di Catania, CT, Italia
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Aggiungi al carrelloVersione per fisarmonica. - in 8° - pp.2 - Brossura editoriale - In buone condizioni - Libro usato.
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Da: Ria Christie Collections, Uxbridge, Regno Unito
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Aggiungi al carrelloCondizione: New. In.
Condizione: New. pp. 370.
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Aggiungi al carrelloTaschenbuch. Condizione: Neu. Physics of Formation of FeII Lines Outside LTE | Proceedings of the 94th Colloquium of the International Astronomical Union Held in Anacapri, Capri Island, Italy, 4-8 July 1986 | Roberto Viotti (u. a.) | Taschenbuch | Astrophysics and Space Science Library | xiii | Englisch | 2014 | Springer | EAN 9789401082853 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.
Da: Revaluation Books, Exeter, Regno Unito
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Aggiungi al carrelloPaperback. Condizione: Brand New. 1988 edition. 368 pages. 10.10x7.10x0.90 inches. In Stock.
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Aggiungi al carrelloTaschenbuch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - The same kind of physics is frequently common to very different fields of Astrophysics, so experts in each of these fields have often much to learn from each others. It was therefore logical that the International Astronomical Union should sponsor a colloquium about an ion which pro duces many spectral lines that can be used as a diagnostic for many sorts of objects, and which may sometimes have a major influence on physical processes occurring in astro physical sources. The lines of singly ionized iron (FeII) are present in absorption and emission in the spectra of objects such as the Sun, cool stars, circumstellar envelopes of hot stars, novae, diffuse nebulae including the supernova remnants, and active galactic nuclei. These lines are very often formed far from LTE, and their interpretation is not easy in view of the complex Grotrian diagram for FeII, and the gaps in the knowledge of various physical parameters. In addition, the density of very strong FeII lines becomes very large in the ultraviolet, and the lines can play a major role in the line blanketing. They need therefore to be taken into account in any energy balance argument.
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Aggiungi al carrelloCondizione: Gut. Zustand: Gut | Sprache: Italienisch | Produktart: Bücher | Keine Beschreibung verfügbar.
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ISBN 10: 9401082855 ISBN 13: 9789401082853
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Aggiungi al carrelloTaschenbuch. Condizione: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The same kind of physics is frequently common to very different fields of Astrophysics, so experts in each of these fields have often much to learn from each others. It was therefore logical that the International Astronomical Union should sponsor a colloquium about an ion which pro duces many spectral lines that can be used as a diagnostic for many sorts of objects, and which may sometimes have a major influence on physical processes occurring in astro physical sources. The lines of singly ionized iron (FeII) are present in absorption and emission in the spectra of objects such as the Sun, cool stars, circumstellar envelopes of hot stars, novae, diffuse nebulae including the supernova remnants, and active galactic nuclei. These lines are very often formed far from LTE, and their interpretation is not easy in view of the complex Grotrian diagram for FeII, and the gaps in the knowledge of various physical parameters. In addition, the density of very strong FeII lines becomes very large in the ultraviolet, and the lines can play a major role in the line blanketing. They need therefore to be taken into account in any energy balance argument. 368 pp. Englisch.
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Aggiungi al carrelloCondizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. The same kind of physics is frequently common to very different fields of Astrophysics, so experts in each of these fields have often much to learn from each others. It was therefore logical that the International Astronomical Union should sponsor a colloqu.
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Aggiungi al carrelloCondizione: New. Print on Demand pp. 370 66:B&W 7 x 10 in or 254 x 178 mm Perfect Bound on White w/Gloss Lam.
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Aggiungi al carrelloCondizione: New. PRINT ON DEMAND pp. 370.
Lingua: Inglese
Editore: Springer, Springer Aug 2014, 2014
ISBN 10: 9401082855 ISBN 13: 9789401082853
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Aggiungi al carrelloTaschenbuch. Condizione: Neu. This item is printed on demand - Print on Demand Titel. Neuware -The same kind of physics is frequently common to very different fields of Astrophysics, so experts in each of these fields have often much to learn from each others. It was therefore logical that the International Astronomical Union should sponsor a colloquium about an ion which pro duces many spectral lines that can be used as a diagnostic for many sorts of objects, and which may sometimes have a major influence on physical processes occurring in astro physical sources. The lines of singly ionized iron (FeII) are present in absorption and emission in the spectra of objects such as the Sun, cool stars, circumstellar envelopes of hot stars, novae, diffuse nebulae including the supernova remnants, and active galactic nuclei. These lines are very often formed far from LTE, and their interpretation is not easy in view of the complex Grotrian diagram for FeII, and the gaps in the knowledge of various physical parameters. In addition, the density of very strong FeII lines becomes very large in the ultraviolet, and the lines can play a major role in the line blanketing. They need therefore to be taken into account in any energy balance argument.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 368 pp. Englisch.