Spectroscopic Variability Associated with Chromospheric Activity: The α Cen System

Bibcode
1986LNP...254..488F
DOI
10.1007/3-540-16763-3_244
Foing, B.; Beckman, J.; Crivellari, L.; Vladilo, G.; Char, S.
Referencia bibliográfica

Cool Stars, Stellar Systems and the Sun, Proceedings of the Fourth Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, Held in Santa Fe, New Mexico, October 16-18, 1985. Lecture Notes in Physics, Vol. 254, edited by Michael Zeilik and David M. Gibson, Springer-Verlag, Berlin Heidelberg New York, 1986., p.488

Fecha de publicación:
0
1986
Número de autores
5
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
A a part of a general chromospheric modelling programme on late-type dwarfs, the authors searched for the spectroscopic variability in chromospheric lines associated with activity. They considered especially the α Centauri system, a very close binary system composed of a G2 V and K1 V dwarfs in order to compare them to the sun. The authors searched for the rotational modulation of the chromospheric lines in order to gain information on the surface distribution of active structures on those dwarfs.
Tipo
Con árbitro

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