Extinction of giant H II regions--star-forming complexes in the galaxies M 33, the LMC, and NGC 2403

Details Extinction of giant H II regions--star-forming complexes in the galaxies M 33, the LMC, and NGC 2403 Extinction of giant H II regions--star-forming complexes in the galaxies M 33, the LMC, and NGC 2403

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995arep...39..281s&link_type=abstract

Astronomy Reports, Volume 39, Issue 3, May 1995, pp.281-283

Astronomy and Astrophysics

Astronomy

Scientific paper

The discrepancies between the extinction of gas emission and that of the starlight in giant H II regions, i.e., in star-forming complexes in the galaxies M 33, the LMC, and NGC 2403, were empirically investigated. The extinction values were determined for 30 stars in eight associations in M 33. An empirical relationship between the extinction of starlight and that of the gas emission in giant H II regions (star- forming complexes in the galaxies under study) was obtained.

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