I discuss recent work on the nature of relativistic winds from Rotation Powered Pulsars, on the physics of how they transport energy from the central compact object to the surrrounding world, and how that energy gets converted into observable synchrotron emission
Except where specific reference is made to the work of others, this work is original and has not bee...
International audienceContext. Rapidly rotating neutron stars blow a relativistic, magnetized wind m...
International audienceContext. Rapidly rotating neutron stars blow a relativistic, magnetized wind m...
After discussion of observational constraints on the nature of the MHD wind coupling between the Cra...
This letter is my progress report for the Astrophysics Theory grant. The first goal of the research ...
In the last decade, the relativistic magnetohydrodynamic (MHD) modelling of pulsar wind nebulae, and...
Session 3: Fundamental Physics with PulsarsNeutron stars lose the bulk of their rotational energy in...
We review current theoretical ideas on pulsar winds and their surrounding nebulae. Relativistic MHD ...
We review current theoretical ideas on pulsar winds and their surrounding nebulae. Relativistic MHD ...
We review current theoretical ideas on pulsar winds and their surrounding nebulae. Relativistic MHD ...
In this contribution we review the recent progress in the modelling of Pulsar Wind Nebulae (PWN). We...
Pulsars emit radiation over an extremely wide frequency range, from radio through gamma. Recently, s...
In this contribution we review the recent progress in the modelling of Pulsar Wind Nebulae (PWN). We...
Abstract. Time dependent numerical simulations show that the anisotropy of the energy flux and a wea...
The energy lost by a rotation-powered pulsar is carried by a relativistic flow containing a mixture ...
Except where specific reference is made to the work of others, this work is original and has not bee...
International audienceContext. Rapidly rotating neutron stars blow a relativistic, magnetized wind m...
International audienceContext. Rapidly rotating neutron stars blow a relativistic, magnetized wind m...
After discussion of observational constraints on the nature of the MHD wind coupling between the Cra...
This letter is my progress report for the Astrophysics Theory grant. The first goal of the research ...
In the last decade, the relativistic magnetohydrodynamic (MHD) modelling of pulsar wind nebulae, and...
Session 3: Fundamental Physics with PulsarsNeutron stars lose the bulk of their rotational energy in...
We review current theoretical ideas on pulsar winds and their surrounding nebulae. Relativistic MHD ...
We review current theoretical ideas on pulsar winds and their surrounding nebulae. Relativistic MHD ...
We review current theoretical ideas on pulsar winds and their surrounding nebulae. Relativistic MHD ...
In this contribution we review the recent progress in the modelling of Pulsar Wind Nebulae (PWN). We...
Pulsars emit radiation over an extremely wide frequency range, from radio through gamma. Recently, s...
In this contribution we review the recent progress in the modelling of Pulsar Wind Nebulae (PWN). We...
Abstract. Time dependent numerical simulations show that the anisotropy of the energy flux and a wea...
The energy lost by a rotation-powered pulsar is carried by a relativistic flow containing a mixture ...
Except where specific reference is made to the work of others, this work is original and has not bee...
International audienceContext. Rapidly rotating neutron stars blow a relativistic, magnetized wind m...
International audienceContext. Rapidly rotating neutron stars blow a relativistic, magnetized wind m...