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The OH (1720 MHz) Supernova Remnant Masers in W28: MERLIN and VLBA Polarization Observations
Ian M. Hoffman, W. M. Goss, C. L. Brogan +1
Full-polarization MERLIN and VLBA observations of the 1720 MHz maser emission from the OH molecule in the supernova remnant W28 are presented. Zeeman splitting (|B| \approx 0.75 mG…
Pulsar Wind Nebulae in EGRET Error Boxes
Mallory S. E. Roberts, Crystal L. Brogan, Bryan M. Gaensler +3
A remarkable number of pulsar wind nebulae (PWN) are coincident with EGRET gamma-ray sources. X-ray and radio imaging studies of unidentified EGRET sources have resulted in the dis…
Ain't No Crab, PWN Got A Brand New Bag: Correlated radio and X-ray Structures in Pulsar Wind Nebulae
Mallory S. E. Roberts, Maxim Lyutikov, Bryan M. Gaensler +3
The traditional view of radio pulsar wind nebulae (PWN), encouraged by the Crab nebula's X-ray and radio morphologies, is that they are a result of the integrated history of their…
OH (1720 MHz) Maser Search Toward the Large Magellanic Cloud
C. L. Brogan, W. M. Goss, J. Lazendic +1
We have carried out a sensitive search for OH (1720 MHz) masers in the Large Magellanic Cloud (LMC) toward five regions using the Australia Telescope Compact Array (ATCA). Our sour…
Physical Conditions in Orion's Veil
N. P. Abel, C. L. Brogan, G. J. Ferland +3
Orion's veil consists of several layers of largely neutral gas lying between us and the main ionizing stars of the Orion nebula. It is visible in 21cm H I absorption and in optical…