Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984abas.symp..266d&link_type=abstract
In its Airborne Astron. Symp. p 266-271 (SEE N85-17848 08-89)
Astronomy and Astrophysics
Astronomy
5
Chemical Composition, Far Infrared Radiation, Infrared Astronomy, Milky Way Galaxy, Nitrogen, Oxygen, Planetary Nebulae, Astronomical Spectroscopy, Concentration (Composition), H Ii Regions, Interstellar Matter, Line Spectra, Nitrogen Ions, Oxygen Ions
Scientific paper
Results from a program of far-infrared observations of oxygen and nitrogen in Galactic planetary nebulae and H II regions are presented and discussed. Results indicate that the N/O abundance increases inward towards the galactic center, with a steep rise at the outer edge of the 5 kpc ring of active star-formation. The N/O abundances in the inner galaxy are about 2 to 3 times higher than in H II regions in the solar neighborhood and outer galaxy.
Dinerstein Harriet L.
Genzel R. L.
Lester Dan
Rubin Robert H.
Watson Dan M.
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