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Millimeter-wave Imaging of Pulsar Wind Nebulae
Published online by Cambridge University Press: 19 July 2016
Abstract
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