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Title:
Standard model atmospheres for A-type stars and non-LTE effects
Authors:
Kubát, Jirí; Korcáková, Daniela
Publication:
The A-Star Puzzle, held in Poprad, Slovakia, July 8-13, 2004. Edited by J. Zverko, J. Ziznovsky, S.J. Adelman, and W.W. Weiss, IAU Symposium, No. 224. Cambridge, UK: Cambridge University Press, 2004., p.13-22
Publication Date:
12/2004
Origin:
CUP
Comment:
ISBN: 0521850185
DOI:
10.1017/S1743921304004326
Bibliographic Code:
2004IAUS..224...13K

Abstract

Analyzing the long-term evolution of active regions (ARs) permits to quantify the link between their atmospheric emission (from optical to X-rays) and the magnetic field. Multi-wavelength studies provide the full story, and not just a snapshot, of the phenomena and they allow us analyze how the atmosphere changes as the field strength decreases (with the dispersion of the AR).

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