Massive star formation in H II galaxies - The presence of Wolf-Rayet stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

22

H Ii Regions, Star Formation, Starburst Galaxies, Wolf-Rayet Stars, Astronomical Catalogs, Metallicity, Stellar Evolution, Stellar Mass, Stellar Spectra

Scientific paper

A systematic search of Wolf-Rayet (WR) features in the spectra of the objects in the Spectroscopic Catalog of H II Galaxies is described. The global detection rate and its possible dependence on metallicity are considered. Properties of the systems with detected WR features are discussed. The apparent lack of WR detection in low-metallicity systems is attributed to the fact that massive stars never reach the WR stage in such media. The SNeII contribution to the Blue Bump is analyzed, and it is concluded that large Blue-Bump luminosities should be expected in regions with SN contamination; therefore, it is not advisable to translate Blue-Bump luminosities into the number of WR stars directly.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Massive star formation in H II galaxies - The presence of Wolf-Rayet stars 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 Massive star formation in H II galaxies - The presence of Wolf-Rayet stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Massive star formation in H II galaxies - The presence of Wolf-Rayet stars will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1787189

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.