Spectroscopy of the magnetic cataclysmic variable 0311-227

Details Spectroscopy of the magnetic cataclysmic variable 0311-227 Spectroscopy of the magnetic cataclysmic variable 0311-227

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...243..567c&link_type=abstract

Astrophysical Journal, Part 1, vol. 243, Jan. 15, 1981, p. 567-575.

Other

17

Binary Stars, Magnetic Stars, Stellar Spectra, Variable Stars, White Dwarf Stars, H Lines, Radial Velocity, Spectral Line Width

Scientific paper

Results are presented from 2 A resolution spectrograms of 2 A 0311-227. Emission line profiles are complex, comprising a broad weak base with velocity amplitude K = 600 km/s in the 81 minute orbit, a narrower main component for which K = 350 km/s, and sharp peaks which split (maximum separation approximately 500 km/s) and merge, at least two times, but probably four times, within the orbit. Measurements of these and other quantities are presented and discussed, together with photometric, X-ray, and polarimetric data, in terms of quadrupole or other field configurations.

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