Results 131 to 140 of about 54,710 (141)

Numerical Hydrodynamics and Magnetohydrodynamics in General Relativity. [PDF]

Living Rev Relativ, 2008
Font JA.
europepmc   +1 more source

Exoplanetary Atmospheres-Chemistry, Formation Conditions, and Habitability. [PDF]

Space Sci Rev, 2016
Madhusudhan N, Agúndez M, Moses JI, Hu Y.   +3 more
europepmc   +1 more source

The Astrobiology Primer v2.0. [PDF]

Astrobiology, 2016
Domagal-Goldman SD, Wright KE, Adamala K, Arina de la Rubia L, Bond J, Dartnell LR, Goldman AD, Lynch K, Naud ME, Paulino-Lima IG, Singer K, Walther-Antonio M, Abrevaya XC, Anderson R, Arney G, Atri D, Azúa-Bustos A, Bowman JS, Brazelton WJ, Brennecka GA, Carns R, Chopra A, Colangelo-Lillis J, Crockett CJ, DeMarines J, Frank EA, Frantz C, de la Fuente E, Galante D, Glass J, Gleeson D, Glein CR, Goldblatt C, Horak R, Horodyskyj L, Kaçar B, Kereszturi A, Knowles E, Mayeur P, McGlynn S, Miguel Y, Montgomery M, Neish C, Noack L, Rugheimer S, Stüeken EE, Tamez-Hidalgo P, Imari Walker S, Wong T.   +48 more
europepmc   +1 more source

Gravitational Waves from Gravitational Collapse. [PDF]

Living Rev Relativ, 2003
Fryer CL, New KC.
europepmc   +1 more source

Some of the next articles are maybe not open access.

Related searches:

Reverberation of the Vela PULSAR WIND NEBULA

Письма в Астрономический журнал: Астрономия и космическая астрофизика, 2023
Transonic (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, K. P. Levenfish, G. A. Ponomaryov   +2 more
openaire   +1 more source

Pulsars and Pulsar Wind Nebulae

2019
When 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   +2 more sources

Neutron Stars, Pulsars, and Pulsar Wind Nebulae [PDF]

, 2020
The 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

2018
The 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   +2 more sources

Introduction to Pulsar Wind Nebulae

2016
Pulsar Wind Nebulae are nebulae of electrons and positrons powered by a central pulsar. In this chapter I give a detailed description of star evolution, centered on the description of supernova remnants, pulsars and pulsar wind nebulae. The basic properties of pulsars are explained, together with the emission mechanisms responsible for the production ...
openaire   +2 more sources

Pulsar Wind Nebula

Science, 2010
openaire   +2 more sources