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2002MNRAS.337..327M - Mon. Not. R. Astron. Soc., 337, 327-331 (2002/November-3)
Two jets from the Orion nebula (M42) `proplyds': kinematics, morphologies and origins.
MEABURN J., GRAHAM M.F. and REDMAN M.P.
Abstract (from CDS):
A `standard' model for jets from young, low-mass stars invokes an accelerating, continuous flow outwards with an opening angle of a few degrees. Here an alternative explanation is suggested which may apply to some, if not all, of the proplyd jets. In this, a `bullet' of dense material is ejected which ploughs through dense circumstellar ambient gas. The decelerating tail of material ablated from the surface of the bullet would be indistinguishable from a continuously emitted jet in current observations.
Abstract Copyright: RAS
Journal keyword(s): line: profiles - stars: winds, outflows - ISM: individual: Orion nebula (M42) - ISM: jets and outflows
Simbad objects: 16
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