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A Spectral Analysis of the Central Component of CTB 80

Published online by Cambridge University Press:  19 July 2016

G. Castelletti ,
G. Dubner ,
K. Golap  and
W. M. Goss
G. Castelletti
Affiliation:
Instituto de Astronomía y Física del Espacio (CONICET, UBA), C.C.67, Suc. 28, 1428 Buenos Aires, Argentina
G. Dubner
Affiliation:
Instituto de Astronomía y Física del Espacio (CONICET, UBA), C.C.67, Suc. 28, 1428 Buenos Aires, Argentina
K. Golap
Affiliation:
National Radio Astronomy Observatory, P.O. Box 0, Socorro, New Mexico 87801, USA
W. M. Goss
Affiliation:
National Radio Astronomy Observatory, P.O. Box 0, Socorro, New Mexico 87801, USA

Abstract

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Based on observations of the extended supernova remnant CTB 80 carried out with the Giant Metrewave Radio Telescope (GMRT, India) at 240 and 618 MHz we have analyzed the spectral behavior of the ∼ 10′ nebula formed near the pulsar PSR B1951+32, finding signatures of the interaction of the pulsar with the surrounding plasma.

Type
Part 4: Pulsar Wind Nebulae and Their Environments
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 211 - 212
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

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