cid 968ca49789e7201f067d4b132bee40c468fdff7b2a619508dcbe5d25f1f64f7b · original · open access · via wikipedia
Title: Polar (star) Authors: Venue: Wikipedia Year: unknown Canonical: wiki:polar-star URL: https://en.wikipedia.org/wiki/Polar_(star) Collector: wikipedia OA: true ABSTRACT In astronomy, a polar is a highly magnetic type of cataclysmic variable (CV) binary star system, originally known as an AM Herculis star after the prototype member AM Herculis. Like other CVs, polars contain two stars: an accreting white dwarf (WD), and a low-mass donor star which is transferring mass to the WD as a result of the WD's gravitational pull, overflowing its Roche lobe. Polars are distinguished from other CVs by the presence of a very strong magnetic field in the WD. Typical magnetic field strengths of polar systems are 10 million to 80 million gauss. The WD in the polar AN Ursae Majoris has the strongest known magnetic field among cataclysmic variables, with a field strength of 230 million gauss.