Emission Lines from Jets in Planetary Nebulae

Details Emission Lines from Jets in Planetary Nebulae Emission Lines from Jets in Planetary Nebulae

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002rmxac..13..139l&link_type=abstract

Emission Lines from Jet Flows, Isla Mujeres, Q.R., México, November 13-17, 2000 (Eds. W. J. Henney, W. Steffen, A. C. Raga, and

Astronomy and Astrophysics

Astronomy

4

Ism: Jets And Outflows, Planetary Nebulae

Scientific paper

Emission line profiles from collimated high-velocity outflows or jets in
planetary nebulae (PNe) have diverse characteristics that indicate the
influence of binary cores and magnetic confinement mechanisms in their
origin. In this contribution, a number of cases are presented that
exemplify the complexity of these outflows in PNe.

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