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Structure of Extended Radio Emission in W50 and its Relation to SS 433

Published online by Cambridge University Press:  04 August 2017

T. Velusamy  and
A. Pramesh Rao
T. Velusamy
Affiliation:
Radio Astronomy Centre(TIFR), Ootacamund, India
A. Pramesh Rao
Affiliation:
Radio Astronomy Centre(TIFR), Ootacamund, India

Extract

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The association of SS 433 with SNR W50 suggests several interesting scenerios for the complex emission features observed in W50. Since W50 lies close to galactic plane (b = −2°.5), it is possible some of these features are just chance superpositions. Several of these are seen in association with diffuse X-rays (Seward et al. 1982) and optical filaments (Zeally et al. 1980). At radio wavelengths W50 has been well studied, at 11 cm (Velusamy and Kundu, 1974; Geldzahler et al. 1980) and at 18 cm (Downes et al. 1981; 1982). In this paper we present new observations at 92 cm (327 MHz).

Type
V. Compact Objects Associated With Supernova Remnants, Pulsars and Neutron Stars
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 465 - 467
Copyright
Copyright © Reidel 1983 

References

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