Three‐dimensional Magnetohydrodynamic Modeling of Planetary Nebulae. II. The Formation of Bipolar and Elliptical Nebulae with Point‐symmetric Structures and Collimated Outflows-Reference-Cited by-同舟云学术

Three‐dimensional Magnetohydrodynamic Modeling of Planetary Nebulae. II. The Formation of Bipolar and Elliptical Nebulae with Point‐symmetric Structures and Collimated Outflows

Published:2000-11-20 Issue:1 Volume:544 Page:336-346
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Garcia‐Segura G.,Lopez J. A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/544/i=1/a=336/pdf

Reference39 articles.

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3. The gas dynamics of H II regions. II - Two-dimensional axisymmetric calculations

4. Calvet, N. 1998, in Accretion Processes in Astrophysical Systems: Some Like It Hot!, ed. S. S. Holt & T. R. Kallman (New York: AIP), 495

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