Zobrazeno 1 - 10
of 1 149
pro vyhledávání: '"J. -P. Zahn"'
Autor:
Judith MARTÍN LUCAS
Publikováno v:
Teoría de la Educación: Revista Interuniversitaria, Vol 32, Iss 1(en-jun), Pp 242-244 (2019)
Externí odkaz:
https://doaj.org/article/c53993bc90de420eb4da7a98e929cf50
Autor:
Georgescu, Adelina
Publikováno v:
Bulletin mathématique de la Société des Sciences Mathématiques de la République Socialiste de Roumanie, 1989 Jan 01. 33(3), 283-283.
Externí odkaz:
https://www.jstor.org/stable/43679844
Akademický článek
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Autor:
J. Guzik, A. V. Tutukov, J. P. Zahn, R. Canal, H. Saio, Cesare Chiosi, G. Michaud, W. A. Dziembowski, Alvio Renzini, G. Vauclair, G. Meynet, Don A. VandenBerg
Publikováno v:
Transactions of the International Astronomical Union. 24:201-218
This report focuses on a few subjects where substantial progress has been achieved during the past three years. Several colleagues were asked to describe what they consider as the highlights in their field, and we are very grateful to them for their
Autor:
Baker, N. H.
Publikováno v:
Journal of Fluid Mechanics; March 1979, Vol. 91 Issue: 2 p400-400, 1p
Akademický článek
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Autor:
J.-P. Zahn
Publikováno v:
EAS Publications Series. 63:245-254
The standard model of stellar structure is unable to account for various observational facts, such as anomalies in the surface composition, and there is now a broad consensus that some extra mixing must occur in the radiation zones, in addition to th
Publikováno v:
Communications in Asteroseismology. 157:195-220
Autor:
J. P. Zahn
Publikováno v:
EAS Publications Series. 39:211-222
Magnetic fields have been detected at the surface of many stars, where they are responsible for various activity phenomena, and presumably they are present also in their deep interior. They channel stellar winds to large distance, thus increasing the
Autor:
J.-P. Zahn
Publikováno v:
EAS Publications Series. 26:49-64
Although it presently includes convective overshoot, microscopic diffusion, gravitational settling and radiative acceleration, the standard model of stellar structure is still unable to account for various observational facts, and there is now a larg