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19972004
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astro-ph2004

The orbital period distribution of wide binary millisecond pulsars

B. Willems, U. Kolb

We present results of a binary population synthesis study on the orbital period distribution of wide binary millisecond pulsars forming through four evolutionary channels. In three…

astro-ph2002

XMM-Newton observations of variability in the X-ray binaries of M31: flares dips and a burst

R. Barnard, U. C. Kolb, J. P. Osborne

The XMM-Newton satellite has made four observations of the core of M31 as part of a survey that will span the entire galaxy. The majority of the X-ray emission is contributed by po…

astro-ph2001

A first look at cataclysmic variable stars from the 2dF QSO survey

T. R. Marsh, L. Morales-Rueda, D. Steeghs +9

The 2dF QSO survey is a spectroscopic survey of 48,000 point-sources selected by colour with magnitudes in the range 18.35 < B < 20.95. Amongst QSOs, white dwarfs, narrow-line gala…

astro-ph2000

Irradiation and mass transfer in low-mass compact binaries

H. Ritter, U. Kolb, Z. -Y. Zhang

We study the reaction of low-mass stars to anisotropic irradiation and its importance for the long-term evolution of compact binaries binaries. We show by means of a simple homolog…

astro-ph1998

The CV Period Minimum

Ulrich Kolb, Isabelle Baraffe

Using improved, up-to-date stellar input physics tested against observations of low-mass stars and brown dwarfs we calculate the secular evolution of low-mass donor CVs, including…

astro-ph1998

Are the red dwarfs in cataclysmic variables main-sequence stars?

K. Beuermann, I. Baraffe, U. Kolb +1

We show that the secondaries in short-period cataclysmic variables with orbital periods hr are close to the solar-abundance main sequence defined by single field stars. In…