Determination of N/O from far-infrared line observations of Galactic H II regions
Measurements of the 52- and 88-micron forbidden O III line ratios and the 57-micron forbidden N III line ratio for six H II regions have been obtained with the NASA Kuiper Airborne Observatory. The derived N/O ratio for most Galactic regions (of about 0.2-0.3) is greater than that obtained by optica...
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Veröffentlicht in: | Astrophys. J.; (United States) 1988-04, Vol.327 (1), p.377-388 |
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Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | Measurements of the 52- and 88-micron forbidden O III line ratios and the 57-micron forbidden N III line ratio for six H II regions have been obtained with the NASA Kuiper Airborne Observatory. The derived N/O ratio for most Galactic regions (of about 0.2-0.3) is greater than that obtained by optical studies, and it exceeds the solar value. Although enhancement of N/O at a galactocentric distance of about 6 kpc may be possible, no evidence is found for an overall linear gradient in N/O with galactocentric distance, suggesting that N-14 is predominantly produced by primary rather than secondary nucleosynthesis. |
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ISSN: | 0004-637X 1538-4357 |
DOI: | 10.1086/166200 |