A long period model for the magnetic star gamma Equulei

Details A long period model for the magnetic star gamma Equulei A long period model for the magnetic star gamma Equulei

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...284..174l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 284, no. 1, p. 174-178

Astronomy and Astrophysics

Astrophysics

31

Linear Polarization, Magnetic Stars, Peculiar Stars, Stellar Magnetic Fields, Stellar Rotation, Stellar Models, Time Series Analysis

Scientific paper

Linear polarimetry has enabled us to observe the rotation of the magnetic axis of the star gamma Equ (nearly 15 deg over the period 1990 - 1993). Thus, the very long rotation period of more than 70 years, suggested by previous authors, is now confirmed in a straightforward way. We propose numerical values for the various parameters which enter the oblique rotator model and we show that they are consistent with all the available data on the magnetism of gamma Equ.

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