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Spectroscopy of Stellar Coronal Sources with the Medium Energy Experiment on EXOSAT

Published online by Cambridge University Press:  12 April 2016

R. Pallavicini ,
L. Pasquini ,
J.H.M.M. Schmitt  and
G. Tagliaferri
R. Pallavicini
Affiliation:
Arcetri Astrophysical Observatory, Florence, Italy
L. Pasquini
Affiliation:
Max-Planck-lnstitut fur Extraterrestrische Physik, Garching, Germany
J.H.M.M. Schmitt
Affiliation:
Max-Planck-lnstitut fur Extraterrestrische Physik, Garching, Germany
G. Tagliaferri
Affiliation:
ESTEC, EXOSAT Observatory, Noordwijk, The Netherlands

Abstract

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We summarize some of the results obtained by spectral analysis of EXOSAT ME observations of stellar coronal sources. We focus on time-resolved spectroscopy of stellar flares and on the determination of the temperature structure of quiescent RS CVn binaries

Type
3. Stellar Coronae
Information
International Astronomical Union Colloquium , Volume 115: High Resolution X-ray Spectroscopy of Cosmic Plasmas , 1990 , pp. 122 - 125
Copyright
Copyright © Cambridge University Press 1990

References

Majer, P., Schmitt, J.H.M.M., Golub, L., Harnden, F.R. Jr. and Rosner, R.: 1986, Ap. J. 300, 360.Google Scholar
Mewe, R., Gronenschild, E.H.B.M. and van den Oord, G.H.: 1985, Astr. Ap. Suppl. 62, 197.Google Scholar
Pallavicini, R., Stella, L. and Tagliaferri, G.: 1988, to be submitted to Astr. Ap.Google Scholar
Pallavicini, R., Tagliaferri, G., Pollock, A., Schmitt, J.H.M.M. and Rosso, C.: 1988, submitted to Astr. Ap.Google Scholar
Paresce, F.: 1984, Astr. J. 89,1022.Google Scholar
Pasquini, L., Schmitt, J.H.M.M. and Pallavicini, R.: 1988, submitted to Astr. Ap.Google Scholar
Raymond, J.C. and Smith, B.W.: 1977, Ap. J. Suppl. 35, 419.Google Scholar
Schmitt, J.H.M.M., Pallavicini, R., Monsignori-Fossi, B.C. and Harnden, F.R. Jr.: 1987, Astr. Ap. 179, 197.Google Scholar
Swank, J.H., White, N.E., Holt, S.S. and Becker, R.H.: 1981, Ap. J. 246, 208.CrossRefGoogle Scholar
Tagliaferri, G., Giommi, P., Angelini, L., Osborne, J.P. and Pallavicini, R.: 1988, Ap. J. Letters 331, L113.CrossRefGoogle Scholar
White, N.E. et al. : 1988, this volume.Google Scholar
White, N.E., Culhane, J.L., Parmar, A.N., Kellet, B.J., Kahn, S., van den Oord, G.H.J, and Kuipers, J.: 1986, Ap. J. 301, 262.Google Scholar
White, N.E. and Peacock, A.: 1988, in X-ray Astronomy with EXOSAT (Pallavicini, R. and White, N.E. eds.), in press.Google Scholar