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Spectroscopic and Photometric Observations of the Magnetic Cataclysmic Variable TX Col
Published online by Cambridge University Press: 12 April 2016
Abstract
Simultaneous photometry and spectroscopy of the Intermediate Polar TX Col were obtained in order to investigate its accretion mode and dynamics. The spectroscopic and photometric power spectra of TX Col are observed to change on relatively short timescales. Spectroscopy reveals a dominant periodicity at the orbital period (5.69 hr) and a spin period of 1909 s in radial velocities, while line equivalent widths show a strong periodicity at the beat period (2106 s). It is the first time that the orbital period has been detected in optical wavelengths.
- Type
- Part 3. A. Accretion Plasma diagnostics - Observations
- Information
- International Astronomical Union Colloquium , Volume 190: Magnetic Cataclysmic Variables , 2004 , pp. 156 - 162
- Copyright
- Copyright © Astronomical Society of the Pacific 2004