Faint X-ray sources in the core of the globular cluster M28

R. Danner, S. R. Kulkarni (), Y. Saito and N. Kawai
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R. Danner: Mathematics and Astronomy 105-24, California Institute of Technology
S. R. Kulkarni: Mathematics and Astronomy 105-24, California Institute of Technology
Y. Saito: Institute of Space and Astronautical Science, 3-1-1 Yoshinodai
N. Kawai: The Institute of Physical and Chemical Research, 2-1 Hirosawa Wako

Nature, 1997, vol. 388, issue 6644, 751-753

Abstract: Abstract Globular clusters, the most ancient stellar groups in our galaxy, are known to contain bright X-ray sources, faint X-ray sources and millisecond pulsars. The bright X-ray sources are neutron stars accreting matter from a companion star1, and the millisecond pulsars are believed to be descendants of these sources2. But the origin of the faint X-ray sources remains unclear. Here we report satellite-based X-ray observations of the globular cluster M28 which reveal two faint X-ray sources; an extended source slightly offset from the centre of the cluster, and a point source. The point source pulsates with the same period as a well-known3,4 3-millisecond pulsar in M28. The nature of the extended source is more puzzling, however, and its spatial and spectral properties permit a range of plausible models. We argue that this source is either a collection of low-luminosity accreting neutron-star binaries or a synchrotron nebula powered by a recent outburst of energy from an unknown source. Sensitive optical and X-ray observations should be able to distinguish between these two possibilities.

Date: 1997
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DOI: 10.1038/41962

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