Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...212l.125t&link_type=abstract
Astrophysical Journal, Part 2 - Letters to the Editor, vol. 212, Mar. 15, 1977, p. L125-L129. NSF-supported research.
Astronomy and Astrophysics
Astrophysics
153
Dwarf Stars, Magnetic Stars, Polarization Characteristics, Stellar Magnetic Fields, X Ray Sources, Circular Polarization, Cyclotron Radiation, Novae, Stellar Rotation, Stellar Spectrophotometry
Scientific paper
Linear and circular polarization observed in the V and I spectral bands reveal the presence of a compact star with a magnetic field of the order of 200 million gauss. Large variations of both polarization states, with a period of 0.128918 days, appear to be caused by rotation of the compact star. Unpolarized radiation observed in the U band suggest that a hot source, companion to the compact star, is unaffected by the magnetic field.
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