Spherically Symmetric Relativistic MHD Simulations of Pulsar Wind Nebulae in Supernova Remnants

Astronomy and Astrophysics - France
doi 10.1051/0004-6361:20030624
Full Text
Abstract

Available in full text

Date
Authors
Publisher

EDP Sciences

Related search

Axially Symmetric Relativistic MHD Simulations of Pulsar Wind Nebulae in Supernova Remnants

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2004English

Pulsar Wind Nebulae in Supernova Remnants

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2001English

Model of Radio Emission From Spherically Symmetric Pulsar Wind Nebulae

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

Pulsar Wind Nebulae Modeling

International Journal of Modern Physics: Conference Series
2014English

The Theory of Pulsar Wind Nebulae

International Journal of Modern Physics: Conference Series
2014English

A Method to Estimate the Cooling Time of Ultra-Relativistic Electrons in Pulsar Wind Nebulae

American Journal of Astronomy and Astrophysics
2015English

Hydrodynamics of Relativistic Pulsar Wind

International Astronomical Union Colloquium
1992English

On the Broadband Synchrotron Spectra of Pulsar Wind Nebulae

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

Neutron Stars in Supernova Remnants

Symposium - International Astronomical Union
2000English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2025 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy