The geometry of the magnetic field of 78 Virginis

Details The geometry of the magnetic field of 78 Virginis The geometry of the magnetic field of 78 Virginis

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...235..915b&link_type=abstract

Astrophysical Journal, Part 1, vol. 235, Feb. 1, 1980, p. 915-924. Research supported by the National Research Council of Canad

Other

14

A Stars, Circular Polarization, Interstellar Magnetic Fields, Line Spectra, Magnetic Field Configurations, Magnetic Stars, Stellar Spectra, Astronomical Photography, Computer Programs, Computerized Simulation, Electrophotometers, High Resolution, Quadrupoles, Zeeman Effect

Scientific paper

High-resolution circular polarization and line profiles, across the Fe II lambda 4520.2 line of 78 Vir, are computer modeled in the framework of the oblique rotator model. The observations are reproduced very well with an inclined dipolar geometry that contains a moderate quadrupolar component. The model found is consistent with all the information we have about the magnetic field of 78 Vir. The oblique rotator model thus appears to have passed another direct test.

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