The magnetic field and period of the AP SI star 108 Aquarii

Details The magnetic field and period of the AP SI star 108 Aquarii The magnetic field and period of the AP SI star 108 Aquarii

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...258..389n&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 258, no. 2, p. 389-396.

Astronomy and Astrophysics

Astrophysics

10

A Stars, Astronomical Photometry, Metallic Stars, Peculiar Stars, Stellar Magnetic Fields, Stellar Rotation, Variable Stars, Radial Velocity, Silicon, Spectral Line Width, Stellar Spectra

Scientific paper

New effective magnetic field observations are presented for the bright Ap star 108 Aqr. A new, unambiguous and more precise rotational period of 3.735239 +/- 0.000024 d is found on the basis of recent Geneva photometry and earlier published y measurements. This period is consistent with the magnetic data, which are distributed on a sinusoidal curve and imply beta = 36 +/- 20 deg.

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