ar X iv : a st ro - p h / 01 01 18 0 v 1 1 1 Ja n 20 01 Kinematic Projecting of Pulsar Profiles

ar X iv : a st ro - p h / 01 01 28 2 v 1 1 7 Ja n 20 01 Evidence for Free Precession in the Pulsar B 1642 − 03

We present an analysis of the timing data of the pulsar B1642−03, collected over a span of 30 years between 1969 and 1999. During this interval, the timing residuals exhibit cyclical changes with amplitude varying from 15 ms to 80 ms and spacing of maxima varying from 3 years to 7 years. Interpretation of these observed cyclical changes in terms of free precession suggests a wobble angle of abo...

ar X iv : a st ro - p h / 06 01 33 7 v 1 1 6 Ja n 20 06 A Radio Pulsar Spinning at 716 Hz Jason

X iv :a st ro -p h/ 06 01 33 7v 1 1 6 Ja n 20 06 A Radio Pulsar Spinning at 716 Hz Jason W. T. Hessels, Scott M. Ransom, Ingrid H. Stairs, Paulo C. C. Freire, Victoria M. Kaspi, and Fernando Camilo Department of Physics, McGill University, Montreal, QC H3A 2T8, Canada NRAO, 520 Edgemont Rd., Charlottesville, VA 22903, USA Department of Physics and Astronomy, University of British Columbia, 6224...

ar X iv : a st ro - p h / 97 01 22 8 v 1 2 9 Ja n 19 97 Large - scale Structures revealed by Wavelet Decomposition 1

ar X iv : a st ro - p h / 01 01 31 5 v 1 1 8 Ja n 20 01 Signal Characteristics from Electromagnetic Cascades in Ice

We investigate the development of electromagnetic cascades in ice using a GEANT Monte Carlo simulation. We examine the Cherenkov pulse that is generated by the charge excess that develops and propagates with the shower. This study is important for the RICE experiment at the South Pole, as well as any test beam experiment which seeks to measure coherent Cherenkov radiation from an electromagneti...

ar X iv : a st ro - p h / 96 01 12 9 v 1 2 3 Ja n 19 96 Is Her X - 1 a strange star

The possible identification of Her X-1 with a strange star (Li et al. 1995) is shown to be incorrect.