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The Diversity of Neutron Stars - Nearby Thermally Emitting Neutron Stars and the Compact Central Objects in Supernova Remnants (Paperback)
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The Diversity of Neutron Stars - Nearby Thermally Emitting Neutron Stars and the Compact Central Objects in Supernova Remnants (Paperback)
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Neutron stars are invaluable tools for exploring stellar death, the
physics of ultra-dense matter, and the effects of extremely strong
magnetic fields. The observed population of neutron stars is
dominated by the >1000 radio pulsars, but there are distinct
sub-populations that, while fewer in number, can have significant
impact on our understanding of the issues mentioned above. These
populations are the nearby, isolated neutron stars discovered by
ROSAT, and the central compact objects in supernova remnants. The
studies of both of these populations have been greatly accelerated
in recent years through observations with the Chandra X-ray
Observatory and the XMM-Newton telescope. First, we discuss radio,
optical, and X-ray observations of the nearby neutron stars aimed
at determining their relation to the Galactic neutron star
population and at unraveling their complex physical processes by
determining the basic astronomical parameters that define the
population---distances, ages, and magnetic fields---the
uncertainties in which limit any attempt to derive basic physical
parameters for these objects. magnetic fields above 1e13 Gauss.
Second, we describe the hollow supernova remnant problem: why many
of the supernova remnants in the Galaxy have no indication of
central neutron stars. We have undertaken an X-ray census of
neutron stars in a volume-limited sample of Galactic supernova
remnants, and from it conclude that either many supernovae do not
produce neutron stars contrary to expectation, or that neutron
stars can have a wide range in cooling behavior that makes many
sources disappear from the X-ray sky.
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