Neon, argon, and chlorine abundance gradients from type II planetary nebulae

Details Neon, argon, and chlorine abundance gradients from type II planetary nebulae Neon, argon, and chlorine abundance gradients from type II planetary nebulae

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.129..353f&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 129, no. 2, Jan. 1987, p. 353-360. Research supported by the Fundacao de A

Astronomy and Astrophysics

Astrophysics

23

Abundance, Argon, Chlorine, Neon, Planetary Nebulae, Stellar Composition, Distance, Galactic Nuclei, Milky Way Galaxy

Scientific paper

Heavy-element abundance gradients derived from type II planetary nebulae
(PN) are studied for the elements neon, argon, and chlorine. As in the
case of helium, oxygen, sulphur, and probably carbon and nitrogen, the
abundance of these elements relative to hydrogen present measurable
radial gradients across the galactic disk.

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