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UV energy distributions of active cool stars

Published online by Cambridge University Press:  25 May 2016

C. Morossi ,
M. Franchini  and
M.L. Malagnini
C. Morossi
Affiliation:
Osservatorio Astronomico di Trieste, Via Tiepolo 11, I-34131, Trieste, Italy
M. Franchini
Affiliation:
Osservatorio Astronomico di Trieste, Via Tiepolo 11, I-34131, Trieste, Italy
M.L. Malagnini
Affiliation:
Dipartimento di Astronomia, Università degli Studi di Trieste, Via Tiepolo 11, I-34131, Trieste, Italy

Abstract

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We present semi-empirical models based on the “minimum-temperature-concept” in order to provide a description of the UV spectra of solar type stars consistent with the observational data.

Type
Stellar Flux Distributions
Information
Symposium - International Astronomical Union , Volume 189: Fundamental Stellar Properties: The Interaction Between Observation and Theory , 1997 , pp. 93 - 96
Copyright
Copyright © Kluwer 1997 

References

Cayrel de Strobel, G. 1996, A&AR 7,243 Google Scholar
Edvardsson, B., Andersen, J., Gustafsson, B., Lambert, D.L., Nissen, P.E., Tomkin, J. 1993, A&A 275, 101 (EAGLNT) Google Scholar
Kurucz, R.L. 1993, CD-ROM 13, ATLAS9 Stellar Atmosphere Programs and 2 km/s Grid (Cambridge: Smithsonian Astrophys. Obs.) (K93) Google Scholar
Malagnini, M.L., Morossi, C., Buser, R., Parthasarathy, M. 1992, A&A 261, 558 Google Scholar
Morossi, C., Franchini, M., Malagnini, M.L., Kurucz, R.L., Buser, R. 1993, A&A 277, 173 Google Scholar
Samain, D. 1979, A&A 74, 225 Google Scholar