Abundances of non-type I planetary nebulae in the LMC

Details Abundances of non-type I planetary nebulae in the LMC Abundances of non-type I planetary nebulae in the LMC

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...279..567d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 279, no. 2, p. 567-571

Astronomy and Astrophysics

Astrophysics

9

Abundance, Astronomical Spectroscopy, Chemical Composition, Interstellar Matter, Magellanic Clouds, Planetary Nebulae, Spectroscopic Analysis, Visible Spectrum, Argon, Atomic Spectra, H Lines, Helium, Nitrogen, Oxygen, Spectrographs, Sulfur

Scientific paper

Spectroscopic observations, plasma diagnostics and chemical composition
of 15 non-type I planetary nebulae (PNe) in the Large Magellanic Cloud
(LMC) are reported. Abundances of He, O, N, S, and Ar are determined and
compared with recently obtained data for nebulae both in the Magellanic
Clouds and in the Galaxy.

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