Variability of the uvby light curves of the magnetic CP star 108 Aquarii
Adelman Saul J.
Open Astronomy · 1999
doi:10.1515/astro-1999-0304 (opens in a new tab)
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Abstract
Light curves based on recent Stromgren uvby observations of the mCP star 108 Aqr show definite changes with respect to published uvby data of this star.This behavior is interpreted as being due to the precession of the rotational axis changing slowly and moderately the observed hemisphere of this star at a given rotational phase.
Abstract licence: CC BY
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