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Archive | 1985

A Comparison of H2252-035/AO PSC and 4U1849-31/V1223 SGR

J. van Paradijs; S. van Amerongen; M. De Kool; M. Pakull; H. J. van der Woerd

From five-colour photometry of the triple-periodic systems H2252-035 and V1223 Sgr, which have very similar orbital and pulsation periods, we find a significant difference in the wavelength dependence of their short period pulsations. Our results indicate that in H2252-035 this pulse originates in a hot region, probably on the white dwarf (Motch and Pakull, 1981), whereas in V1223 Sgr both pulses are the result of reprocessing of X-rays (in the far side of the accretion disk, and in the companion star, respectively), as suggested by Warner (1985).


Monthly Notices of the Royal Astronomical Society | 1986

Accretion from an inhomogeneous medium – III. General case and observational consequences

Mario Livio; Noam Soker; M. De Kool; G. J. Savonije


Monthly Notices of the Royal Astronomical Society | 1986

On accretion of angular momentum from an inhomogeneous medium

Mario Livio; Noam Soker; M. De Kool; G. J. Savonije


Monthly Notices of the Royal Astronomical Society | 1986

Accretion of angular momentum from an inhomogeneous medium – II. Isothermal flow

Noam Soker; Mario Livio; M. De Kool; G. J. Savonije


Astronomy and Astrophysics | 1992

Statistics of cataclysmic variable formation

M. De Kool


Astronomy and Astrophysics | 1993

On the formation rate and space density of close white dwarf main sequence star binaries

M. De Kool; H. Ritter


Monthly Notices of the Royal Astronomical Society | 1984

Photometry of A0538 - 66 during an active and subsequent inactive state

J. van Paradijs; S. van Amerongen; M. De Kool; M. Pakull; E. R. Deul; J. Lub; A. Greve


Astronomy and Astrophysics | 1987

Neutron star spin evolution in wide low-mass X-ray binaries

M. De Kool; J. van Paradijs


Astronomy and Astrophysics | 1994

PG 1416-129: a broad absorption line QSO with low intrinsic X-ray absorption

M. De Kool; E. J. A. Meurs


Astronomy and Astrophysics | 1993

The period distribution of cataclysmic binaries evolving without magnetic braking

Ulrich C. Kolb; M. De Kool

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Mario Livio

Technion – Israel Institute of Technology

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Noam Soker

Technion – Israel Institute of Technology

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M. Pakull

Technical University of Berlin

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J. Lub

European Southern Observatory

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