The cataclysmic variable binary V533 Herculis (Nova 1963)

Details The cataclysmic variable binary V533 Herculis (Nova 1963) The cataclysmic variable binary V533 Herculis (Nova 1963)

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pasp...99...57h&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 99, Jan. 1987, p. 57-61.

Astronomy and Astrophysics

Astronomy

6

Binary Stars, Cataclysmic Variables, Novae, Stellar Spectrophotometry, Abundance, Emission Spectra, Line Spectra, Radial Velocity, Stellar Orbits

Scientific paper

Results are presented of 69 spectra of V533 Her obtained during 1981 - 86. Radial velocities show a large scatter above measuring errors, and a binary period is not uniquely determined. Its most probable value is 0.2097774 day. Binary parameters are not critically dependent on the period and are discussed. Emission lines are weak, and show small but unusual phase modulation. Very weak lines of He I, He II, C II, and N III are detected, preferably at some orbital phases.

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