High-velocity bipolar mass flow in the planetary nebula NGC 2392

Details High-velocity bipolar mass flow in the planetary nebula NGC 2392 High-velocity bipolar mass flow in the planetary nebula NGC 2392

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...295l..17g&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 295, Aug. 1, 1985, p. L17-L20.

Astronomy and Astrophysics

Astrophysics

49

Astronomical Spectroscopy, Planetary Nebulae, Stellar Mass Ejection, Bipolarity, Fabry-Perot Interferometers, H Alpha Line, Symbiotic Stars

Scientific paper

Detailed spectroscopic observations of a high-velocity component in the velocity field of the "Eskimo" nebula, NGC 2392, are presented. It is interpreted as a jetlike multiknot bipolar mass flow with a velocity of nearly 200 km s-1 and a small angle of collimation less than 10°. Electron density, mass, kinetic energy, and power are estimated.

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