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Radio Continuum Observations of Supernova Remnants at 22 GHz

Published online by Cambridge University Press:  12 April 2016

C.E. Tateyama ,
N.S.P. Sabalisck  and
Z. Abraham
C.E. Tateyama
Affiliation:
INPE:Instituto de Pesquisas Espaciais, MCT. C.P. 515, 12.200 Sao José dos Campos, SP, Brazil
N.S.P. Sabalisck
Affiliation:
INPE:Instituto de Pesquisas Espaciais, MCT. C.P. 515, 12.200 Sao José dos Campos, SP, Brazil
Z. Abraham
Affiliation:
INPE:Instituto de Pesquisas Espaciais, MCT. C.P. 515, 12.200 Sao José dos Campos, SP, Brazil

Abstract

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We describe in this work the results of high frequency radio continuum observations of 96 supernova remnants (SNRs) obtained at the Itapetinga Observatory at 22 GHz. We have detected 15 SNRs. Most of the strongest SNRs detected were previously classified in terms of their spectral and morphological properties as filled-center type (Crab-like). Some of the others have doubtful classifications.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 305 - 308
Copyright
Copyright © Cambridge University Press 1988

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