The ISO spectrum of the planetary nebula NGC 6302. II. Nebular abundances

Details The ISO spectrum of the planetary nebula NGC 6302. II. Nebular abundances The ISO spectrum of the planetary nebula NGC 6302. II. Nebular abundances

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26a...347..975p&link_type=abstract

Astronomy and Astrophysics, v.347, p.975-982 (1999)

Astronomy and Astrophysics

Astrophysics

43

Stars: Abundances, Stars: Evolution, Ism: Planetary Nebulae: Individual: Ngc 6302, Infrared: Ism: Lines And Bands

Scientific paper

The ISO spectrum of NGC 6302 is used, in conjunction with the visible and ultraviolet spectrum, to determine the nebular composition. In addition to being considerably more accurate than previous determinations, the abundances of many more elements (and ions) can be found. A discussion of the previous evolution of the central star, in the light of these abundances, is given. A discussion is also given of the composition of the dust.

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