We present a table of 215 supernova remnants (SNRs) with distances. New distances are
found to SNR G51. 26+ 0.11 of 6.6±1.7 kpc using H i absorption spectra and to five other …

Thermonuclear and core-collapse supernova remnants (SNRs) are the nebular leftovers of
defunct stars. Their morphology and emission properties provide insights into the …

The birth properties of neutron stars (NSs) yield important information about the still-debated
physical processes that trigger the explosion as well as on intrinsic neutron-star physics …

Under the assumption that jets explode all core collapse supernovae (CCSNe), I classify 14
CCSN remnants (CCSNRs) into five groups according to their morphology as shaped by …

Supernova explosions are inherently asymmetric and can accelerate new-born neutron
stars (NSs) to hundreds of km s− 1. Two prevailing theories to explain NS kicks are ejecta …

The X-ray emission from a supernova remnant (SNR) is a powerful diagnostic of the state of
the shocked plasma. The temperature (kT) and the emission measure (EM) of the shocked …

Core-collapse supernova remnants are the gaseous nebulae of galactic interstellar media
(ISM) formed after the explosive death of massive stars. Their morphology and emission …

We study the morphologies of core collapse supernova remnants (CCSNRs) and find that
about third of CCSNRs in our sample have two opposite 'ears' protruding from their main …

Context. Central compact objects (CCOs) are a peculiar class of neutron stars, primarily
encountered close to the center of young supernova remnants (SNRs) and characterized by …

The fraction of stars that are in binaries or triples at the time of stellar death and the fraction
of these systems that survive the supernova explosion are crucial constraints for evolution …