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Time-Resolved Spectroscopy and Doppler Tomography of UX UMa

Published online by Cambridge University Press:  22 February 2018

V. F. Suleimanov ,
V. V. Neustroev ,
N. V. Borisov  and
I. S. Fioktistova
V. F. Suleimanov
Affiliation:
Department of Astronomy, Kazan State University, Kremlevskaya str. 18, 120008, Kazan, Russia (vals@ksu.ru)
V. V. Neustroev
Affiliation:
Computational Astrophysics Laboratory, National University of Ireland, Galway, Ireland (benj@it.nuigalway.ie)
N. V. Borisov
Affiliation:
Special Astrophysical Observatory, Russia
I. S. Fioktistova
Affiliation:
Special Astrophysical Observatory, Russia

Extract

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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 Hβ emission line are found to have semi-amplitude of about 100 km/s.

Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 270
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

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