The Pulsar Wind Nebula Around PSR B1853+01 in the Supernova Remnant W44-Reference-Cited by-同舟云学术

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The Pulsar Wind Nebula Around PSR B1853+01 in the Supernova Remnant W44

Published:1996-06-20 Issue:2 Volume:464 Page:L165-L168
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:

Author:

Frail D. A.,Giacani E. B.,Goss W. M.,Dubner G.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference50 articles.

1. Arons, J. 1992, in IAU Colloq. 128, The Magnetospheric Structure and Emission Mechanisms of Radio Pulsars, ed. J. A. Gil, T. H. Hankins, & J. M. Rankin (Zielona Gora: Pedagogical Univ. Press), 56

2. Asymptotic domination of cold relativistic MHD winds by kinetic energy flux

3. Does the VELA pulsar have 'wisps'?

4. Activity and radio spectral index variations near the center of the Crab nebula

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