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Millimeter-wave Imaging of Pulsar Wind Nebulae

Published online by Cambridge University Press:  19 July 2016

Douglas C.-J. Bock  and
Bryan M. Gaensler
Douglas C.-J. Bock
Affiliation:
Radio Astronomy Laboratory, University of California, 601 Campbell Hall, Berkeley, CA 94720, USA
Bryan M. Gaensler
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS-6, Cambridge, MA 02138, USA

Abstract

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We have observed the supernova remnants G16.7+0.1 and G29.7−0.3 at millimeter wavelengths with the Berkeley-Illinois-Maryland Association array, measuring total flux densities of the pulsar wind nebulae in the remnants. Our results imply a break at ∼50 GHz in the spectrum of the PWN in G29.7−0.3, lower than previously estimated. The PWN in G16.7+0.1 either has a break < 100 GHz, or a steep radio spectrum.

Type
Part 4: Pulsar Wind Nebulae and Their Environments
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 207 - 210
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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