A typical SS 433 VLBI radio structure

Details A typical SS 433 VLBI radio structure A typical SS 433 VLBI radio structure

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...189..124f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 189, no. 1-2, Jan. 1988, p. 124-127. ZWO-supported research.

Astronomy and Astrophysics

Astrophysics

6

Radio Stars, Stellar Spectrophotometry, Very Long Base Interferometry, Centimeter Waves, Spectrum Analysis

Scientific paper

VLBI observations of SS433 with the European Network at 18 cm on 15 March 1986 show the source to contain a strong unresolved core, symmetrically placed structure on either side of the core, a sharp cut off at about 100 mas from the core and discontinuous ejection, all features seen in earlier observations. The authors discuss evidence for a brightening zone around SS433 (Vermeulen et al., 1987).

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