Correlated H-alpha and continuum variability of X Persei A

Details Correlated H-alpha and continuum variability of X Persei A Correlated H-alpha and continuum variability of X Persei A

Jul 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.176..233m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 176, July 1976, p. 233-236.

Astronomy and Astrophysics

Astronomy

7

B Stars, Continuous Radiation, Emission Spectra, H Alpha Line, Radiant Flux Density, Absorption Spectra, Astronomical Photometry, Balmer Series, Binary Stars, Flares, X Ray Sources

Scientific paper

An observation is reported which shows a rapid collapse of the H-alpha
emission line in X Per A, associated with a flare in the continuum.
There is some evidence that this anticorrelated variability, occurring
on a time scale of 450 s, is associated with the massive secondary in
the X Per binary system.

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