Series merging of hydrogen Balmer lines during a stellar flare

Details Series merging of hydrogen Balmer lines during a stellar flare Series merging of hydrogen Balmer lines during a stellar flare

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...148..240z&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 148, no. 1, July 1985, p. 240-242.

Astronomy and Astrophysics

Astrophysics

8

Balmer Series, Flare Stars, Stark Effect, Stellar Flares, Stellar Spectra, Chromosphere, Doppler Effect, Hydrogen

Scientific paper

The authors demonstrate that the series merging of Stark broadened hydrogen Balmer profiles can produce a significant and, possibly, observable continuum enhancement in the vicinity of the Balmer jump. They discuss the implications of this result for the enhanced "blue" continuum that is often observed in solar and stellar flares. The results are compared with a flare spectrum obtained for the dMe star YZ CMi.

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