A shadowed flow in the STEM of the Crab nebula?

Details A shadowed flow in the STEM of the Crab nebula? A shadowed flow in the STEM of the Crab nebula?

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985natur.313..661m&link_type=abstract

Nature (ISSN 0028-0836), vol. 313, Feb. 21, 1985, p. 661, 662.

Astronomy and Astrophysics

Astronomy

8

Astronomical Models, Crab Nebula, Flow Stability, Molecular Clouds, Stellar Envelopes, Supernovae, Supersonic Flow

Scientific paper

The faint radio and emission line 'jet' outward from the northern boundary of the Crab Nebula which appears as a neat right cylinder is modelled here as the convected margin of a gas cloud that accidentially cast its shallow across the nearly ballistic flow of the stellar envelope ejected in the supernova explosion. It is shown that this model is consistent with known data on the jet, and that it accounts for the strikingly regular geometrical features in a natural way. In contrast, flow instability models do not easily result in so neat a cylinder.

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