Optical observations of the jet of the Crab Nebula

Details Optical observations of the jet of the Crab Nebula Optical observations of the jet of the Crab Nebula

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...151..101v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 151, no. 1, Oct. 1985, p. 101-104.

Astronomy and Astrophysics

Astrophysics

10

Astronomical Photometry, Crab Nebula, Jets, Supernova Remnants, H Alpha Line, Mass Distribution, Oxygen Spectra

Scientific paper

Photometry of the jet in the Crab Nebula in the forbidden lines of O III and H-alpha + N II is presented. A mass of 0.003 solar masses is estimated for the matter in the jet. The connection of the jet to the filamentary shell suggests that it is due to an instability of the confinement of the relativistic particles and magnetic fields in the Nebula.

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