Pulsars steadily dissipate their rotational energy via relativistic winds. Confinement of these
outflows generates luminous pulsar wind nebulae, seen across the electromagnetic …

Supernova remnants are beautiful astronomical objects that are also of high scientific
interest, because they provide insights into supernova explosion mechanisms, and because …

Massive star supernovae can be divided into four categories, depending on the amount of
mass loss from the progenitor star and the star's radius: red supergiant stars with most of the …

The empirical relation between the X-ray luminosity (in the 2–10 keV band) and the rate of
spin-down energy loss of a sample of 39 pulsars is re-examined considering recent data …

We investigate the relation between the optical extinction (AV) and the hydrogen column
density (NH) determined from X-ray observations of a large sample of Galactic sightlines …

We study observational constraints on neutron star (NS) kicks for isolated pulsars and for
NSs in binary systems. We are particularly interested in the evidence of kick-spin alignment …

We present a detailed radio study of the young supernova remnant (SNR) G292. 0+ 1.8 and
its associated pulsar PSR J1124-5916, using the Australia Telescope Compact Array at …

We report the discovery with the Parkes radio telescope of a pulsar associated with the∼
1700 yr old oxygen-rich composite supernova remnant G292. 0+ 1.8. The pulsar PSR J1124 …

We present a study of the Galactic supernova remnant (SNR) G292. 0+ 1.8, a classic
example of a core-collapse SNR that contains oxygen-rich ejecta, circumstellar material, a …

ABSTRACT Using the High Resolution Camera on board the Chandra X-ray Observatory,
we have re-examined the proper motion of the central compact object RX J0822− 4300 in …