Magnetic Models of HD 115708 and HD 119419

Details Magnetic Models of HD 115708 and HD 119419 Magnetic Models of HD 115708 and HD 119419

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ap.....44...98g&link_type=abstract

Astrophysics (English translation of Astrofizika), v. 44, Issue 1, p. 98-105 (2001).

Astronomy and Astrophysics

Astrophysics

Scientific paper

The magnetic fields of the chemically peculiar stars HD 115708 and HD 119419 were modeled using observed curves of variation of the magnetic field with the phase of the rotational period. It turned out that the field of HD 115708 is described, in a first approximation, by a central dipole, while the field of HD 119419 is described by an off-center dipole. The main parameters of the magnetic fields of both stars and maps of the surface field-strength distribution were obtained. The dipole axis of the first star lies in the equatorial plane while that of the second is almost parallel to the axis of rotation.

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