Add to ORKGIn this brief review, I discuss recent developments in the study of pulsar-powered nebulae ("plerions"). The large volume of data which has been acquired in recent years reveals a diverse range of observational properties, demonstrating how differing environmental and pulsar properties manifest themselves in the resulting nebulae
We present high resolution VLA images taken at the wavelengths of lambda 20 cm, lambda 6 cm, and lam...
The resonant cyclotron absorption model (Hoshino et al. 1992; Gallant & Arons 1994) is very successf...
This letter is my progress report for the Astrophysics Theory grant. The first goal of the research ...
After discussion of observational constraints on the nature of the MHD wind coupling between the Cra...
We review recent theoretical developments on pulsar winds, their nebulae and relativistic shock acce...
I discuss recent work on the nature of relativistic winds from Rotation Powered Pulsars, on the phys...
We present observations with the Chandra X-ray Observatory of the pulsar wind nebula (PWN) powered b...
The Large High Altitude Air Shower Observatory has reported the detection of cosmic-ray sources in M...
Abstract. Time dependent numerical simulations show that the anisotropy of the energy flux and a wea...
In this contribution we review the recent progress in the modelling of Pulsar Wind Nebulae (PWN). We...
The general properties of the nonthermal nonpulsed X-ray emission of rotation-powered pulsars are in...
We report the results of X-ray (Chandra X-ray Observatory (CXO)) and radio (ATCA) observations of th...
We present results from Chandra and XMM-Newton observations pulsar B1046-58. A high-resolution spati...
Session 3: Fundamental Physics with PulsarsNeutron stars lose the bulk of their rotational energy in...
Based on the expected population of core collapse supernova remnants and the huge number of detected...
We present high resolution VLA images taken at the wavelengths of lambda 20 cm, lambda 6 cm, and lam...
The resonant cyclotron absorption model (Hoshino et al. 1992; Gallant & Arons 1994) is very successf...
This letter is my progress report for the Astrophysics Theory grant. The first goal of the research ...
After discussion of observational constraints on the nature of the MHD wind coupling between the Cra...
We review recent theoretical developments on pulsar winds, their nebulae and relativistic shock acce...
I discuss recent work on the nature of relativistic winds from Rotation Powered Pulsars, on the phys...
We present observations with the Chandra X-ray Observatory of the pulsar wind nebula (PWN) powered b...
The Large High Altitude Air Shower Observatory has reported the detection of cosmic-ray sources in M...
Abstract. Time dependent numerical simulations show that the anisotropy of the energy flux and a wea...
In this contribution we review the recent progress in the modelling of Pulsar Wind Nebulae (PWN). We...
The general properties of the nonthermal nonpulsed X-ray emission of rotation-powered pulsars are in...
We report the results of X-ray (Chandra X-ray Observatory (CXO)) and radio (ATCA) observations of th...
We present results from Chandra and XMM-Newton observations pulsar B1046-58. A high-resolution spati...
Session 3: Fundamental Physics with PulsarsNeutron stars lose the bulk of their rotational energy in...
Based on the expected population of core collapse supernova remnants and the huge number of detected...
We present high resolution VLA images taken at the wavelengths of lambda 20 cm, lambda 6 cm, and lam...
The resonant cyclotron absorption model (Hoshino et al. 1992; Gallant & Arons 1994) is very successf...
This letter is my progress report for the Astrophysics Theory grant. The first goal of the research ...