Planetary nebulae in the Magellanic Clouds (2): Features of their chemical abundances

Details Planetary nebulae in the Magellanic Clouds (2): Features of their chemical abundances Planetary nebulae in the Magellanic Clouds (2): Features of their chemical abundances

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.215..285a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 215, no. 2, p. 285-301

Astronomy and Astrophysics

Astrophysics

Abundance, Magellanic Clouds, Milky Way Galaxy, Planetary Nebulae, Stellar Composition, Stellar Evolution, Stellar Mass, Classifications, Cyanides, Data Correlation, Oxygen Compounds

Scientific paper

Using the classification scheme for planetary nebulae in the Magellanic Clouds using four criteria proposed in Paper 1, all nebulae are divided into three classes on the basis of the mass of their central stars. The features of individual chemical abundances in the Magellanic Cloud planetary nebulae and the way in which there differ from the galactic planetary nebulae are investigated separately for each class of nebulae. The role of CN and ON cycling in intermediate mass star evolution is discussed.

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