Results 161 to 170 of about 5,865 (191)
The Evolution of Compact Binary Star Systems. [PDF]
Living Rev Relativ, 2006 Postnov KA, Yungelson LR.
europepmc +1 more source
Very large radio surveys of the sky. [PDF]
Proc Natl Acad Sci U S A, 1999 Condon JJ.
europepmc +1 more source
Magnetic fields in non-convective regions of stars. [PDF]
R Soc Open Sci, 2017 Braithwaite J, Spruit HC.
europepmc +1 more source
Gravitational Waves from Gravitational Collapse. [PDF]
Living Rev Relativ, 2011 Fryer CL, New KC.
europepmc +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Reverberation of the Vela PULSAR WIND NEBULA
Письма в Астрономический журнал: Астрономия и космическая астрофизика, 2023Transonic (withMach numberMs 1) motion of a pulsar relative to the external medium canhelp its compact pulsar wind nebula develop a double-torus X-ray morphology. The double-torus structurecan reverberate as a whole under the dynamic pressure of the external flow. For a flow aligned with thesymmetry axis of the nebula, the response of the double-torus
A. E. Petrov +2 more
openaire +1 more source
Pulsars and Pulsar Wind Nebulae
2019When heavy stars have burned all their nuclear fuel, neutron degeneracy pressure is the last force able to halt their collapse into a black hole. The sudden stop of the free-fall collapse leads to a rebound of the infalling matter triggering an outward shock that blows up the star envelope and powers a Type II supernova.
openaire +1 more source
Neutron Stars, Pulsars, and Pulsar Wind Nebulae
2020The connection between supernovae and neutron stars goes back to the seminal publications by W. Baade and F. Zwicky in 1934, in which they coined both the term “super-nova”, suggested a connection between cosmic rays and “super-novae” and postulated that a “super-nova” event “represents the transition of an ordinary star into a neutron star”.
openaire +1 more source
Introduction to Pulsar Wind Nebulae
2018The ejected material by a SN explosion interacts with the surrounding environment, giving rise to a new astrophysical object known as SNR (for a review of this matter, I refer the reader to (Reynolds 2008) and to Appendix A for more information on the first evolutionary phase).
openaire +1 more source