Time-resolved spectroscopy and Doppler tomography of UX UMa

Details Time-resolved spectroscopy and Doppler tomography of UX UMa Time-resolved spectroscopy and Doppler tomography of UX UMa

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004rmxac..20..270s&link_type=abstract

Compact Binaries in the Galaxy and Beyond, Proceedings of the conference held 17-22 November, 2003 in La Paz, Baja California Su

Astronomy and Astrophysics

Astronomy

3

Novae, Cataclysmic Variables, Stars: Individual (Ux Uma)

Scientific paper

Medium resolution spectroscopy of nova-like cataclysmic variable UX UMA was performed using the 6-m telescope SAO RAS in April 1999. Obtained spectra cover the total orbital period including eclipse phases and allow us to reproduce the radial velocity curve. The radial-velocity variations of the H β emission line are found to have semi-amplitude of about 100 km/s.

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