RX J0944.5+0357: A Probable Intermediate Polar
arXiv:astro-ph/0301594 · doi:10.1023/B:ASTR.0000005092.30409.81
Abstract
From optical photometry the cataclysmic variable RX J0944.5+0357 is shown to have a double-peaked pulse profile with a period of ~2160 s. The two peaks vary rapidly in relative amplitude. Often most of the optical power is concentrated in the first harmonic of the 2160s modulation: RX J0944.5+0357 therefore probably belongs to the relatively rare class of two-pole accreting intermediate polars exemplified by YY Dra and V405 Aur.
8 pages, 5 figures; accepted for publication by Astrophysics and Space Science