Evolving radio structure of the binary star SS433 at a resolution of 15 MARC S

Details Evolving radio structure of the binary star SS433 at a resolution of 15 MARC S Evolving radio structure of the binary star SS433 at a resolution of 15 MARC S

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987natur.328..309v&link_type=abstract

Nature (ISSN 0028-0836), vol. 328, July 23, 1987, p. 309-313. ZWO-supported research.

Computer Science

49

Binary Stars, Stellar Evolution, Stellar Motions, Stellar Spectrophotometry, Stellar Structure, Very Long Base Interferometry, Data Reduction, Radio Spectra, Stellar Mass Ejection

Scientific paper

A comprehensive series of VLBI (very-long-baseline interferometry)
observations of SS433, carried out over an 11-day period on the European
VLBI Network at 5 GHz, reveals the motion and evolution of a series of
faint 'blobs' ejected from the system. These blobs are observed to
brighten at a substantial distance from the binary star.

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