Numerical simulations of the collision of an inhomogeneous stellar wind and a relativistic pulsar wind in a binary system

Binary systems hosting a massive star and a non-accreting pulsar present strong interacting winds. The stellar wind can be clumpy resulting in an unstable two-wind interaction region, which can strongly influence the non-thermal emission of the binary system. We performed axisymmetric relativistic h...

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Autores principales: Paredes-Fortuny, Xavier, Bosch-Ramon,Valentí, Perucho, Manel, Ribó, Marc
Formato: Objeto de conferencia
Lenguaje:Inglés
Publicado: 2015
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/167943
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id I19-R120-10915-167943
record_format dspace
spelling I19-R120-10915-1679432024-07-11T20:03:01Z http://sedici.unlp.edu.ar/handle/10915/167943 Numerical simulations of the collision of an inhomogeneous stellar wind and a relativistic pulsar wind in a binary system Paredes-Fortuny, Xavier Bosch-Ramon,Valentí Perucho, Manel Ribó, Marc 2015-10 2016 2024-07-11T13:26:26Z en Ciencias Astronómicas relativistic pulsar wind inhomogeneous stellar wind axisymmetric relativistic hydrodynamical simulations Binary systems hosting a massive star and a non-accreting pulsar present strong interacting winds. The stellar wind can be clumpy resulting in an unstable two-wind interaction region, which can strongly influence the non-thermal emission of the binary system. We performed axisymmetric relativistic hydrodynamical simulations of the interaction between a relativistic pulsar wind (Lorentz factors up to 6) and an inhomogeneous stellar wind with different degrees of inhomogeneity. The simulations show that the stellar wind inhomogeneities can significantly reduce the two-wind interaction region size. In addition, the whole interaction region is quite unstable, and presents a complex spatial and temporal pattern, with the shocked pulsar wind structure strongly changing under small perturbations. All of this can lead to strong variations in the non-thermal output from these binary systems. Facultad de Ciencias Astronómicas y Geofísicas Objeto de conferencia Objeto de conferencia http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf 87-92
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
relativistic pulsar wind
inhomogeneous stellar wind
axisymmetric relativistic hydrodynamical simulations
spellingShingle Ciencias Astronómicas
relativistic pulsar wind
inhomogeneous stellar wind
axisymmetric relativistic hydrodynamical simulations
Paredes-Fortuny, Xavier
Bosch-Ramon,Valentí
Perucho, Manel
Ribó, Marc
Numerical simulations of the collision of an inhomogeneous stellar wind and a relativistic pulsar wind in a binary system
topic_facet Ciencias Astronómicas
relativistic pulsar wind
inhomogeneous stellar wind
axisymmetric relativistic hydrodynamical simulations
description Binary systems hosting a massive star and a non-accreting pulsar present strong interacting winds. The stellar wind can be clumpy resulting in an unstable two-wind interaction region, which can strongly influence the non-thermal emission of the binary system. We performed axisymmetric relativistic hydrodynamical simulations of the interaction between a relativistic pulsar wind (Lorentz factors up to 6) and an inhomogeneous stellar wind with different degrees of inhomogeneity. The simulations show that the stellar wind inhomogeneities can significantly reduce the two-wind interaction region size. In addition, the whole interaction region is quite unstable, and presents a complex spatial and temporal pattern, with the shocked pulsar wind structure strongly changing under small perturbations. All of this can lead to strong variations in the non-thermal output from these binary systems.
format Objeto de conferencia
Objeto de conferencia
author Paredes-Fortuny, Xavier
Bosch-Ramon,Valentí
Perucho, Manel
Ribó, Marc
author_facet Paredes-Fortuny, Xavier
Bosch-Ramon,Valentí
Perucho, Manel
Ribó, Marc
author_sort Paredes-Fortuny, Xavier
title Numerical simulations of the collision of an inhomogeneous stellar wind and a relativistic pulsar wind in a binary system
title_short Numerical simulations of the collision of an inhomogeneous stellar wind and a relativistic pulsar wind in a binary system
title_full Numerical simulations of the collision of an inhomogeneous stellar wind and a relativistic pulsar wind in a binary system
title_fullStr Numerical simulations of the collision of an inhomogeneous stellar wind and a relativistic pulsar wind in a binary system
title_full_unstemmed Numerical simulations of the collision of an inhomogeneous stellar wind and a relativistic pulsar wind in a binary system
title_sort numerical simulations of the collision of an inhomogeneous stellar wind and a relativistic pulsar wind in a binary system
publishDate 2015
url http://sedici.unlp.edu.ar/handle/10915/167943
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AT boschramonvalenti numericalsimulationsofthecollisionofaninhomogeneousstellarwindandarelativisticpulsarwindinabinarysystem
AT peruchomanel numericalsimulationsofthecollisionofaninhomogeneousstellarwindandarelativisticpulsarwindinabinarysystem
AT ribomarc numericalsimulationsofthecollisionofaninhomogeneousstellarwindandarelativisticpulsarwindinabinarysystem
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