High resolution profiles of Balmer lines in four late type dwarfs.

Details High resolution profiles of Balmer lines in four late type dwarfs. High resolution profiles of Balmer lines in four late type dwarfs.

Sep 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997pobeo..57...61j&link_type=abstract

Publications of the Astronical Observatory of Belgrade, No. 57, p. 61 - 65

Astronomy and Astrophysics

Astronomy

Late-Type Dwarfs: Balmer Lines

Scientific paper

The authors present high resolution spectra of the first five Balmer lines in four late type dwarfs (CR Dra, CN Leo, CE Boo and BY Dra) observed during the night of 22/23 May 1997. Strong self-reversals are detected in Hα and Hδ line in all stars. They have determined the equivalent width of the observed Balmer lines which indicate that the position of the transition region of these stars lies at around log m = -4.

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