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astro-ph2008

IP Pegasi in outburst: Echelle spectroscopy & Modulation Doppler Tomography

C. Papadaki, H. M. J. Boffin, D. Steeghs

We analyse a unique set of time-resolved echelle spectra of the dwarf nova IP Peg, obtained at ESO's NTT with EMMI. The dataset covers the wavelength range of 4000-7500A and shows…

astro-ph20082 cited

Photometric study of selected cataclysmic variables II. Time-series photometry of nine systems

C. Papadaki, H. M. J. Boffin, V. Stanishev +3

We present time-series photometry of nine cataclysmic variables: EI UMa, V844Her, V751 Cyg, V516 Cyg, GZ Cnc, TY Psc, V1315 Aql, ASAS J002511+1217.12, V1315 Aql and LN UMa. The obs…

astro-ph2004

Simultaneous Doppler maps of IP Peg in outburst

C. Papadaki, H. M. J. Boffin, D. Steeghs

IP Pegasi is an eclipsing dwarf nova lying above the period gap with an orbital period of 3.8h. It is the first cataclysmic variable to show evidence of spiral arms in its accretio…

astro-ph2004

Gas flow in close binary star systems

K. Oka, T. Matsuda, I. Hachisu +1

We first present a summary of our numerical work on accretion discs in close binary systems. Our recent studies on numerical simulations of the surface flow on the mass-losing star…

astro-ph2003

Time-resolved photometry of cataclysmic variables

C. Papadaki, H. M. J. Boffin, J. Cuypers +3

We present time-resolved photometry of two cataclysmic variables whose CCD photometric observations were obtained with the 1m telescope at the South African Astronomical Observator…

astro-ph2003

HD 112914 : A nearby one solar mass binary system

Henri M. J. Boffin, Dimitri Pourbaix

In paper 167 of his serie published in The Observatory, Griffin presented the spectroscopic orbit of HD 112914, a late main sequence star. He also noticed that this star, also know…