9780792340270 - Stellar Surface Structure (International Astronomical Union Symposia, 176, Band 176) (4 Ergebnisse)

Zustand: New. In.

Couverture souple. Zustand: bon. R260269821: 1996. In-8. Broché. Très bon état, Couv. convenable, Dos satisfaisant, Intérieur frais. 598 pages augmentées de quelques figures et photos en noir et blanc dans texte. . . . Classification Dewey : 420-Langue anglaise. Anglo-saxon.

Zustand: New. Proceedings of the 176th Symposium of the International Astronomical Union, held in Vienna, Austria, October 9-13, 1995 Editor(s): Strassmeier, Klaus G.; Linsky, Jeffrey L. (National Institute of Standards and Technology). Series: International Astronomical Union Symposia (Closed). Num Pages: 624 pages, biography. BIC Classification: PGS; PHVB. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 234 x 156 x 32. Weight in Grams: 873. . 1996. 1996th Edition. paperback. . . . . Books ship from the US and Ireland.

Taschenbuch. Zustand: Neu. Neuware - In the past decade, indirect (Doppler) imaging techniques have opened up a whole new discipline in stellar astronomy, providing increasingly detailed photometric, magnetic, and chemical inhomogeneity images of stellar surfaces. Furthermore, new optical interferometers are already being used with sophisticated interferometer techniques to image stellar surface structures more directly, and in the future the ESO VLT Interferometer and other instruments will extend these capabilities enormously. These developments are highlighted in the first two sections of this book. The large number of recent results, ground-based and space-based, and the lack of a generally accepted dynamo theory with predictive power for the stars and the Sun, result in an ever-growing complexity of interpretation of individual results. The IAU Symposium 176 on `Stellar Surface Structure' consequently focused on spatially resolved stellar observations throughout the H-R diagram, from O- and B-stars to late M-stars. Two further sections in this book summarize the current observational data on surface inhomogeneities in stellar photospheres, chromospheres, and coronae. Finally, a special section is devoted to next generation model atmospheres.