Browsing by Subject "X-ray binary stars"
Now showing 1 - 2 of 2
Results Per Page
Sort Options
- ItemOpen AccessQPOs in cataclysmic variables and in X-ray binaries(2005) Kluźniak, W; Lasota, J-P; Abramowicz, M A; Warner, BRecent observations, reported by Warner and Woudt, of Dwarf Nova Oscillations (DNOs) exhibiting frequency drift, period doubling, and 1:2:3 harmonic structure, can be understood as disc oscillations that are excited by perturbations at the spin frequency of the white dwarf or of its equatorial layers. Similar quasi-periodic disc oscillations in black hole low-mass X-ray binary (LMXB) transients in a 2:3 frequency ratio show no evidence of frequency drift and correspond to two separate modes of disc oscillation excited by an internal resonance. Just as no effects of general relativity play a role in white dwarf DNOs, no stellar surface or magnetic field effects need be invoked to explain the black hole QPOs.
- ItemOpen AccessUnveiling the nature of INTEGRAL objects through optical spectroscopy: III. Observations of seven southern sources(2006) Masetti, N; Pretorius, M L; Palazzi, E; Bassani, L; Bazzano, A; Bird, A J; Charles, P A; Dean, A J; Malizia, A; Nkundabakura, P; Stephen, J B; Ubertini, P. The detection, thanks to the