The development of different analytical and approximate numerical methods for calculations
of shock-wave propagation in the inhomogeneous interstellar medium is reviewed. The …

Near the surface of any neutron star there is a thin heat blanketing envelope that produces
substantial thermal insulation of warm neutron star interiors and that relates the internal …

A new classification of neutron star cooling scenarios, involving either" minimal" cooling or"
enhanced" cooling, is proposed. The minimal cooling scenario replaces and extends the so …

Technological advances in radio telescopes and X-ray instruments over the last 20 years
have greatly increased the number of known supernova remnants (SNRs) and have led to a …

Ages and thermal luminosities of neutron stars, inferred from observations, can be
interpreted with the aid of the neutron star cooling theory to gain information on the …

A catalogue of supernova remnants in the southern Galaxy within the area, has been
produced from observations made at 0.843 GHz with a resolution of using the Molonglo …

When I started working on my PhD project on X-ray spectroscopy of supernova remnants in
1995, one of the things that I missed was a good textbook covering the various aspects of …

We perform a combined analysis of the recent AMS-02 data on electrons, positrons,
electrons plus positrons and positron fraction, in a self-consistent framework where we …

Abstract We observed 1E 1207.4-5209, a neutron star in the center of the supernova
remnant PKS 1209-51/52, with the ACIS detector aboard the Chandra X-Ray Observatory …

Context. Over the past five decades, radio astronomy has shown that molecular complexity
is a natural outcome of interstellar chemistry, in particular in star forming regions. However …