2 research outputs found
Partial Replacement of Dietary Animal Protein with Vegetable Protein Blend with Different Proportions of Glucosamine on Growth, Feed Efficiency, Body Composition and Survival of Fingerlings of Asian Catfish (Clarias batrachus)
Neutron Stars and Black Holes in X-ray Binaries
Galactic accretion driven stellar X-ray sources can be divided into groups in
different ways. An important division, which covers almost all known X-ray
binaries, can be made according to the mass of the donor star: high-mass X-ray
binaries and low-mass X-ray binaries. Another distinction (partially
overlapping with the previous one) can be made on the basis of the nature of
the accreting object: a strongly magnetized neutron star, a neutron star with a
weak magnetic field, or a black hole. In this review I describe the properties
of these different types of X-ray binaries, and discuss the mass determinations
which are the basis for distinguishing accreting neutron stars from black
holes.Comment: 58 pages, 15 figures. To be published in 'The Many Faces of Neutron
Stars', R. Buccheri, J. van Paradijs, M.A. Alpar (Eds), Kluwer Academic
Publisher