Magnetohydrodynamic models of bipolar knotty jet in henize 2-90

Lee, C.; Sahai,  R.

dc.contributor.author	Lee, C.	en_US
dc.contributor.author	Sahai, R.	en_US
dc.date.accessioned	2004-09-16T17:53:53Z
dc.date.available	2004-09-16T17:53:53Z
dc.date.issued	2004-05	en_US
dc.identifier.citation	Astrophysical journal, vol. 606, pp. 483-496	en_US
dc.identifier.clearanceno	04-0562	en_US
dc.identifier.uri	http://hdl.handle.net/2014/6191
dc.description.abstract	A remarkably linear, bipolar, knotty jet was recently discovered in Hen 2-90, an object classified as a young planetary nebula. Using two-dimensional, magnetohydrodynamic simulations, we investigate periodic variations in jet density and velocity as the mechanism for producing the jet and its knotty structures.	en_US
dc.format.extent	838580 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en_US
dc.subject.other	bipolar stars winds outflows jet density	en_US
dc.title	Magnetohydrodynamic models of bipolar knotty jet in henize 2-90	en_US