33 citations · 33 across the 1 of their papers we have counts for
6 papers
A Proper Motion for the Pulsar Wind Nebula G359.23-0.82, "the Mouse," Associated with the Energetic Radio Pulsar J1747-2958
C. A. Hales, B. M. Gaensler, S. Chatterjee +2
The "Mouse" (PWN G359.23-0.82) is a spectacular bow shock pulsar wind nebula, powered by the radio pulsar J1747-2958. The pulsar and its nebula are presumed to have a high space ve…
Magneto-rotational overstability in accretion disks
J. W. S. Blokland, E. van der Swaluw, R. Keppens +1
We present analytical and numerical studies of magnetorotational instabilities occuring in magnetized accretion disks. In these studies we make use of the linearised compressible M…
An evolutionary model for pulsar-driven supernova remnants
E. van der Swaluw, T. P. Downes, R. Keegan
We present a model of a pulsar wind nebula evolving inside its associated supernova remnant. The model uses a hydrodynamics code to simulate the evolution of this system when the p…
Interaction of High-Velocity Pulsars with Supernova Remnant Shells
E. van der Swaluw, A. Achterberg, Y. A. Gallant +2
Hydrodynamical simulations are presented of a pulsar wind emitted by a supersonically moving pulsar. The pulsar moves through the interstellar medium or, in the more interesting ca…
Proper Motion Measurements of Pulsar B1951+32 in the Supernova Remnant CTB 80
J. M. Migliazzo, B. M. Gaensler, D. C. Backer +3
Using the Very Large Array and the Pie Town antenna, we have measured the position of the radio pulsar B1951+32 relative to nearby background radio sources at four epochs between 1…
Inferring Initial Spin Periods for Neutron Stars in Composite Remnant
Eric van der Swaluw, Yanqin Wu
We propose a method to infer the initial spin period of pulsars residing in composite supernova remnants. Such a remnant consists of both a plerionic and a shell type component, co…