Computer Science
Scientific paper
Oct 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010xmm..prop..146k&link_type=abstract
XMM-Newton Proposal ID #06735101
Computer Science
White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Her X-1
Scientific paper
A continuous monitoring of the neutron star spin period in Her X-1 and its X-ray luminosity performed with Swift/BAT over the last five years revealed unexpected behavior of the pulsar that appears to switch between two different regimes of the angular momentum exchange between the neutron star and accretion disc. A smooth spin-up of the neutron star is occasionally interrupted by short and strong spin-down episodes accompanied with drops in the X-ray flux. The authors of the proposal recently suggested that such episodes are likely associated with strong outflow of matter from the inner parts of the accretion disc along the opened magnetic field lines which might play an important role in all Roche lobe overflowing X-ray binaries. With the proposed observations we
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