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 |