A search for cyclotron lines in the optical spectra of novalike stars - Preliminary results

Details A search for cyclotron lines in the optical spectra of novalike stars - Preliminary results A search for cyclotron lines in the optical spectra of novalike stars - Preliminary results

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980sval....6...87v&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Mar. 1980, p. 159-165.) Soviet Astronomy Letters, vol. 6, Mar.-Apr. 1980, p. 87-90.

Astronomy and Astrophysics

Astronomy

9

Binary Stars, Cyclotron Radiation, Dwarf Stars, Late Stars, Novae, Stellar Spectra, Brightness, Magnetic Stars, Plasma Waves, Spectral Line Width

Scientific paper

The emission features observed in the spectra of AM Her at 4550-4610 A
and of MV Lyr near 4200 A may be interpreted as electron cyclotron
lines. The degenerate dwarf components of these binary systems would
then have surface magnetic fields of 2.3 + or - 0.1 x 10 to the 8th and
2.6 + or - 0.2 x 10 to the 8th gauss.

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