Extinction characteristics of giant HII regions - Star-forming complexes in the galaxies M33, LMC, and NGC 2403

Details Extinction characteristics of giant HII regions - Star-forming complexes in the galaxies M33, LMC, and NGC 2403 Extinction characteristics of giant HII regions - Star-forming complexes in the galaxies M33, LMC, and NGC 2403

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995azh....72..318s&link_type=abstract

Astronomicheskij Zhurnal, vol. 72, p. 318

Statistics

Computation

7

Spiral Galaxies, H Ii Regions, Star Formation, Magellanic Clouds, Emission Spectra, Outgassing, Computational Astrophysics, Semiempirical Equations

Scientific paper

The discrepancies between the extinction of gas emission and that of the starlight in giant HII regions, star-forming complexes in the galaxies M33, LMC, and NGC 2403, were empirically investigated. The extinction values were determined for 30 stars in eight associations in M33. An empirical relation between the extinction of starlight and that of the gas emission in giant HII regions, star-forming complexes in the galaxies under study, was obtained.

Affiliated with

Also associated with

No associations

Rating

Extinction characteristics of giant HII regions - Star-forming complexes in the galaxies M33, LMC, and NGC 2403 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Extinction characteristics of giant HII regions - Star-forming complexes in the galaxies M33, LMC, and NGC 2403, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Extinction characteristics of giant HII regions - Star-forming complexes in the galaxies M33, LMC, and NGC 2403 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1203379