On the abundance of sulphur in H II regions

Details On the abundance of sulphur in H II regions On the abundance of sulphur in H II regions

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.183p...1p&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 183, Apr. 1978, p. 1P-4P.

Astronomy and Astrophysics

Astronomy

16

Abundance, H Ii Regions, Magellanic Clouds, Photoionization, Sulfur, Electron Density (Concentration), Ionization Cross Sections

Scientific paper

Sulfur abundances determined from the forbidden S III line at 6312 A using the currently favored ionization correction procedure in Orion and in the H II regions of the Magellanic Clouds show a marked trend with the degree of ionization measured by O(++)/O. An explanation is suggested and used to propose an improved ionization correction scheme. The abundance ratio of sulfur to oxygen in both LMC and SMC H II regions is about the same as in Orion.

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