Mhd models for pne
Fuente:
Redalyc
Saved in:
| Main Author: | |
|---|---|
| Format: | Artículo científico |
| Language: | en |
| Published: |
Universidad Nacional Autónoma de México
2000
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1876435961094602752 |
|---|---|
| author | M. Rózyczka |
| author_facet | M. Rózyczka |
| contents | Mhd models for pne M. Rózyczka N. Langer J. Franco G. García Segura J. A. López Física, Astronomía y Matemáticas MHD ISM: JETS AND OUTFLOWS PLANETARY NEBULAE: GENERAL A self-consistent scenario to explain the morphology of planetary nebulae ispresented. This scenario is consistent with the Galactic distribution of di erentnebular types. This work addresses several controversial features that appear inplanetary nebulae, which are easily solved by the inclusion of MHD e ects. Thesefeatures include the presence of axisymmetric and collimated outows with linearlyincreasing kinematics, and the existence of asymmetrical morphologies suchas point-symmetric nebulae. 2000 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57100951 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.9 |
| format | Artículo científico |
| id | redalyc_57100951 |
| institution | Redalyc |
| language | en |
| publishDate | 2000 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | Mhd models for pne M. Rózyczka Física, Astronomía y Matemáticas MHD ISM: JETS AND OUTFLOWS PLANETARY NEBULAE: GENERAL Mhd models for pne M. Rózyczka N. Langer J. Franco G. García Segura J. A. López Física, Astronomía y Matemáticas MHD ISM: JETS AND OUTFLOWS PLANETARY NEBULAE: GENERAL A self-consistent scenario to explain the morphology of planetary nebulae ispresented. This scenario is consistent with the Galactic distribution of di erentnebular types. This work addresses several controversial features that appear inplanetary nebulae, which are easily solved by the inclusion of MHD e ects. Thesefeatures include the presence of axisymmetric and collimated outows with linearlyincreasing kinematics, and the existence of asymmetrical morphologies suchas point-symmetric nebulae. 2000 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57100951 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.9 |
| title | Mhd models for pne |
| topic | Física, Astronomía y Matemáticas MHD ISM: JETS AND OUTFLOWS PLANETARY NEBULAE: GENERAL |
| url | https://www.redalyc.org/articulo.oa?id=57100951 |