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Analysis of Ca II emission lines in seven RSCVn systems

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Fernández Figueroa, María José and Montesinos, B. and Castro Rubio, Elisa de and Rego Fernández, Manuel and Giménez, A. and Reglero, V. (1986) Analysis of Ca II emission lines in seven RSCVn systems. Astronomy & Astrophysics, 169 (01-feb). pp. 219-226. ISSN 0004-6361

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Official URL: http://adsabs.harvard.edu/abs/1986A%26A...169..219F


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Abstract

We report here new Ca II H and K emission line fluxes and equivalent widths for seven RSCVn binary systems, observed at several orbital phases. All the stars show enhanced chromospheric activity. With information from available spectra, an in­ dividual study for each star has been done. Double emission has been found for some systems in which perhaps the hotter compo­nent could be the more active. We have tested spectroscopically the model of localized active regions for the prototype RSCVn.


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© European Southern Observatory.
© EDP Sciencies
The Isaac Newton Telescope, on the island of La Palma, is operated by the Royal Greenwich Observatory at the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. We are grateful to the VILSPA staff for the use of their facil­ities. We thank Dr. R. González Riestra and Dr. J. Zamorano for help with IHAP use. The authors are indebted to an anonymous referee for his critical reading of the manuscript and valuable comments. This work has been supported by the Spanish Comisión Asesora de Investigación Científica y Técnica (CAICYT No. 2254/83).

Uncontrolled Keywords:RSCVn binaries; Chromospheric activity; Ca II emission
Subjects:Sciences > Physics > Astrophysics
Sciences > Physics > Astronomy
ID Code:32756
Deposited On:26 Aug 2015 12:50
Last Modified:10 Dec 2018 15:05

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