Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003newar..47..629l&link_type=abstract
New Astronomy Reviews, Volume 47, Issue 6-7, p. 629-632.
Astronomy and Astrophysics
Astronomy
25
Scientific paper
Detailed analysis of HST and VLA observations enables quantitative modeling of the internal structure of the kiloparsec-scale jet in M87. The jet transverse profiles can be modeled by double-Gaussian profiles. The jet structure is dominated by two threads resembling closely a double helix visible until about 20'' distance. It is produced by a combination of the helical mode and of the elliptical mode of Kelvin-Helmholtz instability. The elliptical mode dominates the pre-knot A jet, while the helical mode becomes prominent at larger distances. Modeling the jet structure constrains well the instability pattern speed, βw=0.5c and jet viewing angle, θj=40°. The estimated bulk Lorentz factor of the jet is 3.4. The model reproduces the jet structure on scales of up to 50'' (accounting for the jet curvature).
Eilek Jean
Hardee Philip
Lobanov Andrei
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