Abstract
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.
Guest investigator at the Hale Observatories, Astronomical Institute of Catania University.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Similar content being viewed by others
Reference
Blanco, C., Catalano, S., Marilli, E., and Rodonò, M.: 1974, Astron. Astrophys. 33, 257.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1976 IAU
About this chapter
Cite this chapter
Blanco, C., Catalano, S., Marilli, E. (1976). Absolute Fluxes of K Chromospheric Emission on the H-R Diagram. In: Bumba, V., Kleczek, J. (eds) Basic Mechanisms of Solar Activity. International Astronomical Union / Union Astronomique Internationale, vol 71. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-1481-6_40
Download citation
DOI: https://doi.org/10.1007/978-94-010-1481-6_40
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-277-0681-2
Online ISBN: 978-94-010-1481-6
eBook Packages: Springer Book Archive