The dwarf nova CZ ORI in outburst

Details The dwarf nova CZ ORI in outburst The dwarf nova CZ ORI in outburst

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...281..808s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 281, no. 3, p. 808-810

Astronomy and Astrophysics

Astrophysics

4

Cataclysmic Variables, Dwarf Novae, Orbital Elements, Visible Spectrum, Astronomical Spectroscopy, Emission Spectra, H Beta Line, Radial Velocity, Stellar Mass

Scientific paper

We present optical spectroscopic observations of the Dwarf Nova CZ Ori during maximum and decline phase of an outburst. Radial velocity measurements reveal an orbital period of (0.2147 +/- 0.0002) days. A valuation of the primary and secondary star masses, together with orbital inclination are given utilizing Roche geometry and accretion disk theory.

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