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High Time Resolution Photometry of Red Dwarf Flare Stars I. A Search For Fine Structures on the Optical Light Curves of Flares

Published online by Cambridge University Press:  27 September 2017

G.M. Beskin
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, 357147 USSR
S.N. Mitronova
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, 357147 USSR
S.I. Neizvestnyj
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, 357147 USSR
V.L. Plakhotnichenko
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, 357147 USSR
L.A. Pustil'nik
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, 357147 USSR
V.F. Shvartsman
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, 357147 USSR
R.E. Gershberg
Affiliation:
Crimean Astrophysical Observatory, Crimea, Nauchny, 334413 USSR

Abstract

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A detailed analysis of 73 flares on UV Cet type stars observed at the 6 m telescope of the Special Astrophysical Observatory with 3x10–7 s time resolution shows no fine structures on flare light curves with time scales from 10–6 to 10–1 s.

Type
Session I: Stellar Flares
Copyright
Copyright © Kluwer 1989

References

Neizvestnyj, S.I., Pimonov, A.A.: 1978, Comm. Special Astrophys. Obs. 23, 56.Google Scholar
Pimonov, A.A.: 1979, Comm. Special Astrophys. Obs. 25, 31.Google Scholar
Plakhotnichenko, V.L.: 1983, Comm. Special Astrophys. Obs. 38, 29.Google Scholar
Shvartsman, V.F.: 1977, Comm. Special Astrophys. Obs. 19, 5.Google Scholar