Hst/uv Periodic Variations in the Intermediate Polar FO AQR

Details Hst/uv Periodic Variations in the Intermediate Polar FO AQR Hst/uv Periodic Variations in the Intermediate Polar FO AQR

Mar 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998balta...7..293s&link_type=abstract

Baltic Astronomy, v.7, p.293-298.

Astronomy and Astrophysics

Astronomy

Stars: Cataclysmic Variables, Intermediate Polars, Individual: Fo Aqr

Scientific paper

A preliminary analysis of high temporal HST UV spectroscopy, as well as SAAO BVRI photometry, has revealed that FO Aqr, differently from all previous observations, has changed from a spin dominated to an orbital dominated variability, both in lines and continuum. The spectral dependence of the orbital continuum, however, has not changed with time. The periodical variations are discussed in terms of standard accretion models.

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