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From Bipolar to Elliptical: Simulating the Morphological Evolution of Planetary Nebulae
From Bipolar Elliptical: Simulating Morphological Evolution Planetary Nebulae
2011/9/27
The majority of Proto-planetary nebulae (PPN) are observed to have bipolar morphologies. The majority of mature PN are observed to have elliptical shapes. In this paper we address the evolution of PPN...
Bipolar clump ejection from a moving source。
Properties of Bipolar Planetary Nebulae。
Fabry-perot kinematics of hh 202-204 in the orion nebula：are they part of a big bipolar outflow?
Fabry-perot kinematics orion nebula hh 202-204
2009/6/10
Fabry-perot kinematics of hh 202-204 in the orion nebula：are they part of a big bipolar outflow?
Bipolar relativistic ejections in Cygnus X-3。