The velocity structure of the supernova remnant N 157 B

Details The velocity structure of the supernova remnant N 157 B The velocity structure of the supernova remnant N 157 B

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...140..390g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 140, no. 2, Nov. 1984, p. 390-392.

Astronomy and Astrophysics

Astrophysics

3

Radio Spectra, Stellar Mass Ejection, Stellar Structure, Supernova Remnants, Velocity Distribution, X Ray Spectra, Crab Nebula, Hydrogen Clouds, Molecular Clouds, Red Shift, Stellar Spectrophotometry

Scientific paper

The supernova remnant N 157 B has been likened to the Crab Nebula on the
basis of its X-ray and radio spectral characteristics. Velocity data are
presented suggesting that, like the Crab, N 157 B is expanding as a
prolate spheroid.

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