9780792307716 - "Flare Stars in Star Clusters, Associations and the Solar Vicinity": Proceedings of the 137th Symposium of the International Astronomical Union Held ... U.s.s.r., O... (12 risultati)

Condizione: New. In.

Condizione: New. Proceedings of the 137th Symposium of the International Astronomical Union, held in Byurakan (Armenia), USSR, October 23-27, 1989 Editor(s): Mirzoyan, L. V.; Pettersen, B. R. (Institute of Theoretical Astrophysics, University of Oslo, Norway); Tsvetkov, M. K. Series: International Astronomical Union Symposia (Closed). Num Pages: 410 pages, biography. BIC Classification: PGS. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 297 x 210 x 24. Weight in Grams: 1390. . 1990. Paperback. . . . .

Condizione: New. pp. 432.

Taschenbuch. Condizione: 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 | Einband - flex.(Paperback) | Englisch | 1990 | Springer Netherland | EAN 9780792307716 | Verantwortliche Person für die EU: Springer Netherlands, Haberstr. 7, 69126 Heidelberg, buchhandel-buch[at]springer[dot]com | Anbieter: preigu.

Condizione: New. Proceedings of the 137th Symposium of the International Astronomical Union, held in Byurakan (Armenia), USSR, October 23-27, 1989 Editor(s): Mirzoyan, L. V.; Pettersen, B. R. (Institute of Theoretical Astrophysics, University of Oslo, Norway); Tsvetkov, M. K. Series: International Astronomical Union Symposia (Closed). Num Pages: 410 pages, biography. BIC Classification: PGS. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 297 x 210 x 24. Weight in Grams: 1390. . 1990. Paperback. . . . . Books ship from the US and Ireland.

Taschenbuch. Condizione: 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. Condizione: 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.

Taschenbuch. Condizione: Neu. This item is printed on demand - it takes 3-4 days longer - 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. 436 pp. Englisch.

Kartoniert / Broschiert. Condizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Proceedings of the 137th Symposium of the International Astronomical Union, held in Byurakan (Armenia), USSR, October 23-27, 1989 Stellar flares represent one of the most challenging problems of contemporary astrophysics. Both solar and stellar observ.

Condizione: New. Print on Demand pp. 432 2:B&W 6 x 9 in or 229 x 152 mm Perfect Bound on Creme w/Gloss Lam.

Condizione: New. PRINT ON DEMAND pp. 432.

Taschenbuch. Condizione: Neu. This item is printed on demand - Print on Demand Titel. 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.