Keywords
Bipolar Nebulae:Planetary Nebulae
Planetary Nebulae:Bipolar Nebulae
Planetary Nebulae:Element Abundances
Planetary Nebulae:Progenitors
Planetary Nebulae:Bipolar Nebulae
Planetary Nebulae:Element Abundances
Planetary Nebulae:Progenitors
How to Cite
Bipolar nebulae and Type I planetary nebulae. (1980). Revista Mexicana De Astronomía Y Astrofísica, 5(1), 319-328. https://astronomia.unam.mx/journals/rmxaa/article/view/1983rmxaa...5..319c
Abstract
It is suggested that the bipolar nature of PN of Type I can be explained in terms of their relatively massive progenitors (M ≥ 2.4 M_sun;), that had to lose an appreciable fraction of their mass and angular momentum during their planetary nebula stage. The following objects are discussed in relation with this suggestion: NGC 6302, NGC 2346, NGC 2440, CRL 618, Mz-3 and M2-9.Similar Articles
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