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Absolute Fluxes of K Chromospheric Emission on the H-R Diagram

Published online by Cambridge University Press:  14 August 2015

C. Blanco ,
S. Catalano  and
E. Marilli
C. Blanco
Affiliation:
Catania Astrophysical Observatory and Astronomical Institute, University of Catania, Italy
S. Catalano
Affiliation:
Catania Astrophysical Observatory and Astronomical Institute, University of Catania, Italy
E. Marilli
Affiliation:
Catania Astrophysical Observatory and Astronomical Institute, University of Catania, Italy

Abstract

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Continuing our previous analysis of the chromospheric emission (Blanco et al., 1974), absolute fluxes of the K emission line have been evaluated from 10 Å mm−1 spectrograms of the O. C. Wilson collection for 31 F5-K7 main sequence stars and 172 G2-M5 giants.

Type
Part 4: Stellar Activity of the Solar Type
Information
Symposium - International Astronomical Union , Volume 71: Basic Mechanisms of Solar Activity , 1976 , pp. 473
Copyright
Copyright © Reidel 1976 

References

Blanco, C., Catalano, S., Marilli, E., and Rodonò, M.: 1974, Astron. Astrophys. 33, 257.Google Scholar