The characteristics of the cool component of the cataclysmic binary AE Aquarii derived from its HIPPARCOS parallax

Details The characteristics of the cool component of the cataclysmic binary AE Aquarii derived from its HIPPARCOS parallax The characteristics of the cool component of the cataclysmic binary AE Aquarii derived from its HIPPARCOS parallax

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997newa....2..319f&link_type=abstract

New Astronomy, vol. 2, no. 4, p. 319-322.

Astronomy and Astrophysics

Astronomy

17

Stars: Individual: Ae Aqr, Novae, Cataclysmic Variables

Scientific paper

Observations of the parallax of the cataclysmic binary AE Aqr, using the HIPPARCOS satellite, are combined with the published spectrum and magnitudes in the K band. The radius of the cool component of the binary is probably significantly larger than that of a main sequence star of the same spectral type, though the errors and uncertainties do not make this result completely certain.

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