3D hydrodynamical models of point-symmetric planetary nebulae: the special case of H 1-67
Author:
Affiliation:
1. Instituto de Astronomía, Universidad Nacional Autónoma de México, Apdo. Postal 70264, 04510, Ciudad de México, México
2. Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Apdo. Postal 70543, 04510, Ciudad de México, México
Funder
Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México
Consejo Nacional de Ciencia y Tecnología
European Space Agency
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/482/1/1163/26206283/sty2758.pdf
Reference52 articles.
1. Quantitative classification of WR nuclei of planetary nebulae
2. The evolution of planetary nebulae. I - Structures, ionizations, and morphological sequences
3. NGC 6543: The Rings Around the Cat’s Eye
4. A Survey of Planetary Nebulae in the Southern Galactic Bulge
5. An Interacting Binary System Powers Precessing Outflows of an Evolved Star
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