Planetary nebulae in the Magellanic Clouds (1): Classification and mass-dependence of evolution

Details Planetary nebulae in the Magellanic Clouds (1): Classification and mass-dependence of evolution Planetary nebulae in the Magellanic Clouds (1): Classification and mass-dependence of evolution

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.215..263a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 215, no. 2, p. 263-283

Astronomy and Astrophysics

Astrophysics

Classifications, Comparison, Magellanic Clouds, Milky Way Galaxy, Planetary Nebulae, Stellar Evolution, Abundance, Electron Density Profiles, Expansion, Mathematical Models, Stellar Composition, Stellar Mass, Stellar Temperature, Velocity

Scientific paper

A classification scheme for planetary nebulae (PN) in the Magellanic Clouds using four key criteria is suggested. All nebulae can then be divided into three classes. The features of physical parameters and evolution of the Magellanic Cloud planetary nebulae and the way in which they differ from galactic planetary nebulae are investigated separately for each class of nebulae.

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