Gl 425, a slowly rotating BY Dra-type star.

Details Gl 425, a slowly rotating BY Dra-type star. Gl 425, a slowly rotating BY Dra-type star.

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985rmxaa..10..329t&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, Vol. 10, Spec. issue, p. 329 - 332

Astronomy and Astrophysics

Astrophysics

8

By Draconis Stars:Stellar Flares, By Draconis Stars:Stellar Rotation, Stellar Flares:By Draconis Stars, Stellar Rotation:By Draconis Stars

Scientific paper

The authors observed both components with an intensified Reticon detector at the Cassegrain spectrograph of 1.6 m telescope of the Brazilian Astrophysical Observatory. The brighter component has a filled-in Hα line and the faint companion is a typical dMe star. A spectral classification of dM0e and dM4e is proposed for the pair. An intense flare of Gl 425 was found, indicating that in this aspect it behaves like a normal BY Dra star.

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