Model Nebulae and Determination of the Chemical Composition of the Magellanic Clouds

Details Model Nebulae and Determination of the Chemical Composition of the Magellanic Clouds Model Nebulae and Determination of the Chemical Composition of the Magellanic Clouds

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pnas...76.1525a&link_type=abstract

Proceedings of the National Academy of Sciences of the United States of America, Volume 76, Issue 4, pp. 1525-1528

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18

Scientific paper

An analysis of previously presented photo-electric spectrophotometry of HII regions (emission-line diffuse nebulae) in the two Magellanic Clouds is carried out with the aid of theoretical nebular models, which are used primarily as interpolation devices. Some advantages and limitations of such theoretical models are discussed. A comparison of the finally obtained chemical compositions with those found by other observers shows generally a good agreement, suggesting that it is possible to obtain reliable chemical compositions from low excitation gaseous nebulae in our own galaxy as well as in distant stellar systems.

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