Complex flows in the outer regions of NGC 6302. II

Details Complex flows in the outer regions of NGC 6302. II Complex flows in the outer regions of NGC 6302. II

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.193..631m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 193, Nov. 1980, p. 631-640.

Astronomy and Astrophysics

Astronomy

56

Magnetohydrodynamic Flow, Nebulae, Stellar Mass Ejection, Stellar Winds, Filaments, Radial Velocity, Stellar Temperature

Scientific paper

The motions and densities of the outer filamentary regions of the nebula
NGC 6302 are considered. Many separate volumes of ionized material with
heliocentric radial velocities between -186 and +140 km/sec have been
discovered. Wind driven flows of radiatively ionized material are
proposed to explain these phenomena.

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