mirzoyan l v (7 Ergebnisse)

No Binding. Zustand: Very Good. ORIGINAL reprint/offprint/Extrait of journal article; no covers issued; ex-library; disbound from larger publication; o/w in very good condition. Journal.

gebundene Ausgabe. Zustand: Gut. 444 Seiten; Das hier angebotene Buch stammt aus einer teilaufgelösten wissenschaftlichen Bibliothek und trägt die entsprechenden Kennzeichnungen (Rückenschild, Instituts-Stempel.). Schnitt und Einband sind etwas staubschmutzig; Einbandkanten sind leicht bestossen; der Buchzustand ist ansonsten ordentlich und dem Alter entsprechend gut. Sprache: Englisch Gewicht in Gramm: 950.

Taschenbuch. Zustand: Neu. Flare Stars in Star Clusters, Associations and the Solar Vicinity | Proceedings of the 137th Symposium of the International Astronomical Union Held in Byurakan (Armenia), U.S.S.R., October 23-27, 1989 | L. V. Mirzoyan (u. a.) | Taschenbuch | xx | Englisch | 1990 | Springer Netherland | EAN 9780792307716 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.

Taschenbuch. Zustand: Neu. Neuware -Stellar flares represent one of the most challenging problems of contemporary astrophysics. Both solar and stellar observations have shown the flare phenomenon to be very complex, and in recent years important progress has been made from simultaneous observations over wide wavelength ranges. Some similarities exist between solar and stellar flares, but im portant differences have also been established. Such topics, as well as theoretical aspects, were discussed in detail at the Palo Alto IAU Colloquium No. 104, Solar and Stellar Flares, in 1988. Another approach to the study of stellar flares is through observations of flare stars in physical systems. The possibility of detecting flare stars in star clusters and associations with wide angle telescopes have allowed observations of systems with quite different ages. The classical works of G. Haro and V. A. Ambartsumian demonstrated the evolutionary nature of the flare phenomenon. Flares occur at the earliest stages of dwarf star evolution. The photographic observations of flare stars in systems of different ages turned out to be significant not only for the evolutionary study of flare stars, but also for the study of their physical nature. This observational fact was conditioned by very large diversity of flare star luminosities, i.e. of scales of flares produced by them and by peculiarities of stellar flares observed in star clusters and associations.Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 436 pp. Englisch.

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - Stellar flares represent one of the most challenging problems of contemporary astrophysics. Both solar and stellar observations have shown the flare phenomenon to be very complex, and in recent years important progress has been made from simultaneous observations over wide wavelength ranges. Some similarities exist between solar and stellar flares, but im portant differences have also been established. Such topics, as well as theoretical aspects, were discussed in detail at the Palo Alto IAU Colloquium No. 104, Solar and Stellar Flares, in 1988. Another approach to the study of stellar flares is through observations of flare stars in physical systems. The possibility of detecting flare stars in star clusters and associations with wide angle telescopes have allowed observations of systems with quite different ages. The classical works of G. Haro and V. A. Ambartsumian demonstrated the evolutionary nature of the flare phenomenon. Flares occur at the earliest stages of dwarf star evolution. The photographic observations of flare stars in systems of different ages turned out to be significant not only for the evolutionary study of flare stars, but also for the study of their physical nature. This observational fact was conditioned by very large diversity of flare star luminosities, i.e. of scales of flares produced by them and by peculiarities of stellar flares observed in star clusters and associations.

Couverture souple. Zustand: bon. R260269797: 1990. In-8. Broché. Très bon état, Couv. convenable, Dos satisfaisant, Intérieur frais. 410 pages augmentées de quelques figures en noir et blanc dans texte. . . . Classification Dewey : 420-Langue anglaise. Anglo-saxon.

Couverture rigide. Zustand: Très bon. Jaquette. Edition originale. Armenian Academy of Sciences, Yerevan, 1978. 1st edition. Hardcover, 4to, 444 pages, illustrated with b/w plates and figures. Full blue cloth binding, gilt spine titles, with printed dust jacket. A collections of papers (in Russian, English, French), all published in its original language and with their Russian and English. Contributors: H. Alfven, H. Arp, R. Bellman, A. Blaauw, K.-H. Bohm,B.J. Bok, Ch. Fehrenbach, G.H. Herbig, B. Lovell, L.V. Mirzoyan, E.R. Mustel, J. Neyman, J.H. Oort, Ch. H. Papas, J.-C. Pecker, A.B. Severny, V.V. Sobolev, H.M. Tovmassian, H.-J. Treder, E. Ye. Khachikian, E.G. Yanovitskij. DJ rubbed along edges, with some chipping to spine ends. Binding and pages are clean. A fine copy of a rather scarce book. *//* Académie Arménienne des Sciences, Erevan, 1978. 1ère édition. Cartonnage in-4, 444 pp, illustrées de planches h-t. et des figures en n&b. Reliure pleine toile bleue, dos avec titre doré, avec sa jaquette. Une collection d'articles (en Russe, Anglais, Français), tous publiés dans leur langue originale et suivis de leur traduction en Russe et Anglais. Jaquette frottée, avec signes d'usage. Livre en excellent état. - Weight / Poids livre : 1002 g, ép. 28 mm. ** France LIVRAISON par défaut STANDARD: livraison en RELAIS COLIS Chronopost. PRIORITAIRE: livraison à domicile en Colissimo ou Lettre suivie ++ Selon le POIDS et la VALEUR, nous sommes susceptibles d'AJUSTER à la hausse ou à la baisse les frais de port // Depending on item's WEIGHT or VALUE, we may request Extra Charges, or reduce Shipping Costs **. Livre.