Abstract
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).
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