Pulsar - Supernova Remnant Project Research Interests

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Поисковые слова: massive stars

This page is incomplete. We are endeavouring to make it as complete as possible.

J. G. (Jon) Ables (ATNF)

M. (Matthew) Bailes (ATNF)

L. T. (Lewis) Ball (RCfTA)

J. F. (Jon) Bell (MSSSO)

D. (Douglas) Bock (Astrophysics, Univ. Sydney)

F. M. (Fernando) Camilo (NRAL Jodrell Bank)

D. (Duncan) Campbell-Wilson (Molonglo Observatory, Univ. Sydney)

J. L. (James) Caswell (ATNF)

N. (Nichi) D'Amico (CNR Bologna)

R. (Roy) Duncan (Physics, Univ. Queensland)

B. M. (Bryan) Gaensler (Astrophysics, Univ. Sydney)

A. J. (Anne) Green (Astrophysics, Univ. Sydney)

R. F. (Raymond) Haynes (ATNF)

S. (Simon) Johnston (RCfTA, Univ. Sydney)

V. M. (Vicky) Kaspi (IPAC/JPL/Caltech)

M. J. (Mike) Kesteven (ATNF)

B. S. (Bärbel) Koribalski (ATNF)

S. R. (Shri) Kulkarni (Caltech)

D. R. (Duncan) Lorimer (NRAL Jodrell Bank)

Q. H. Luo (RCfTA, Univ. Sydney)

A. G. (Andrew) Lyne (NRAL Jodrell Bank)

J. N. (Jose') Navarro (NRAO AOC)

D. (Dave) McConnell (ATNF)

R. N. (Dick) Manchester (ATNF)
Most aspects of pulsars. Particular interests in large-scale surveys for pulsars and related population studies, timing observations and their implications for pulsar evolution, pulse shape and polarisation studies and the pulse emission process, use of pulsars as probes of circumstellar gas (especially in PSR J0045-7319 and PSR B1259-63) and the interstellar medium. Origin and evolution of supernova remnants, especially SNR 1987A, and the reasons for barrel-shaped and bi-annular radio morphologies.

D. B. (Don) Melrose (RCfTA, Univ. Sydney)

D. K. (Doug) Milne (Honorary Fellow, ATNF)

J. E. (John) Reynolds (ATNF)

J. S. (Jagmit) Sandhu (Caltech)

B. W. (Ben) Stappers (MSSSO)

L. (Lister) Staveley-Smith (ATNF)

A. K. (Tasso) Tzioumis (ATNF)

M. A. (Mark) Walker (RCfTA, Univ. Sydney)

J. M. (Joel) Weisberg (Carleton College)

M. D. (Matthew) Young (Physics, Univ. of West Australia)

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Last updated on 07-Nov-95 - Dick Manchester (rmanches@atnf.csiro.au)