Investigation of micro-flaring and secular and quasi-periodic variations in dMe flare stars. V - Coronal electrodynamic coupling and the low-activity, M4 dwarf, Gliese 588

Details Investigation of micro-flaring and secular and quasi-periodic variations in dMe flare stars. V - Coronal electrodynamic coupling and the low-activity, M4 dwarf, Gliese 588 Investigation of micro-flaring and secular and quasi-periodic variations in dMe flare stars. V - Coronal electrodynamic coupling and the low-activity, M4 dwarf, Gliese 588

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...235..264a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 235, no. 1-2, Aug. 1990, p. 264-276. Research supported by the European Southe

Astronomy and Astrophysics

Astrophysics

8

Dwarf Stars, Flare Stars, M Stars, Stellar Coronas, Stellar Flares, Variable Stars, Astronomical Photometry, Helioseismology, Periodic Variations, Starspots, Stellar Activity, Stellar Models

Scientific paper

Methods previously used in searches for quasi-periodicities in active dwarf Me flare stars have been applied to the low-activity, dM4 star, Gliese 588. No definite quasi-periodicity was found in the range from about 20 s to a few minutes using three analytical techniques. The implications of these results are given in the context of the Ionson-Mullan senario of coronal heating in late-type dwarfs.

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