P
P. M. McCulloch
Researcher at University of Tasmania
Publications - 176
Citations - 4959
P. M. McCulloch is an academic researcher from University of Tasmania. The author has contributed to research in topics: Pulsar & Very-long-baseline interferometry. The author has an hindex of 37, co-authored 176 publications receiving 4789 citations. Previous affiliations of P. M. McCulloch include Hobart Corporation.
Papers
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Journal ArticleDOI
A Warped Accretion Disk and Wide-Angle Outflow in the Inner Parsec of the Circinus Galaxy
Lincoln J. Greenhill,Roy Booth,Simon Ellingsen,J. R. Herrnstein,J. R. Herrnstein,David L. Jauncey,P. M. McCulloch,James M. Moran,Ray P. Norris,John Reynolds,Anastasios Tzioumis +10 more
TL;DR: In this paper, the first VLBI maps of H2O maser emission (λ 1.3 cm) in the nucleus of the Circinus galaxy, constructed from data obtained with the Australia Telescope Long Baseline Array, were presented.
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Relativistic motion in a nearby bright X-ray source
Steven Tingay,David L. Jauncey,Robert A. Preston,John Reynolds,David L. Meier,David W. Murphy,Anastasios Tzioumis,D. J. McKay,Michael Kesteven,James E. J. Lovell,D. Campbell-Wilson,S. P. Elllngsen,R. G. Gough,Richard W. Hunstead,D. L. Jonos,P. M. McCulloch,Victor Migenes,J. F. H. Quick,M. W. Sinclair,Derck P. Smits +19 more
TL;DR: In this paper, the authors reported high-resolution radio observations of a second Galactic superluminal radio source GRO J1655-40, which was detected as an X-ray transient on 27 July 1994.
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The Vela Pulsar’s Proper Motion and Parallax Derived from VLBI Observations
TL;DR: In this article, the Vela pulsar was derived from 2.3 and 8.4 GHz very long baseline interferometry (VLBI) observations and the data span 6.8 years and consist of 11 epochs.
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The Vela glitch of Christmas 1988
TL;DR: In this article, the Vela pulsar PSR 0833-45 has undergone several large, discontinuous changes (glitches) in its pulsation period and the first time a glitch has been caught as it happened.
Journal ArticleDOI
Overview and initial results of the very long baseline interferometry space observatory programme
Hisashi Hirabayashi,Haruto Hirosawa,Hideyuki Kobayashi,Yasuhiro Murata,P. G. Edwards,Ed Fomalont,Kenta Fujisawa,Tsutomu Ichikawa,Tsuneo Kii,James E. J. Lovell,G. A. Moellenbrock,R. Okayasu,Makoto Inoue,N. Kawaguchi,Seiji Kameno,Kazunori M. Shibata,Y. Asaki,T. Bushimata,S. Enome,Shigeki Horiuchi,Takeshi Miyaji,Tomofumi Umemoto,Victor Migenes,Kiyoaki Wajima,Junichi Nakajima,Masaki Morimoto,J. Ellis,David L. Meier,D. W. Murphy,Robert A. Preston,J. R. Smith,Steven Tingay,D. L. Traub,R. Wietfeldt,J. M. Benson,Mark J. Claussen,Chris Flatters,Jonathan D. Romney,James S. Ulvestad,L. R. D'Addario,Glen Langston,Anthony H. Minter,B. Carlson,Peter E. Dewdney,D. L. Jauncey,John Reynolds,A. R. Taylor,P. M. McCulloch,Wayne Cannon,Leonid I. Gurvits,A. J. Mioduszewski,Richard Schilizzi,Roy Booth +52 more
TL;DR: VSOP images of the gamma-ray source 1156+295, the quasar 1548+056, the ultraluminous quasar 0014+813, and the superluminal quasar 0212+735 are presented and discussed.