Spectral evolutionary synthesis models of metal-poor star forming regions

Details Spectral evolutionary synthesis models of metal-poor star forming regions Spectral evolutionary synthesis models of metal-poor star forming regions

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26as...80..317o&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 80, no. 3, Nov. 1989, p. 317-372.

Astronomy and Astrophysics

Astrophysics

57

Compact Galaxies, Star Formation, Stellar Models, Stellar Spectra, Asymptotic Giant Branch Stars, H Ii Regions, Metallicity, Pre-Main Sequence Stars, Red Giant Stars, Supergiant Stars

Scientific paper

Results are presented from spectral evolutionary synthesis modeling of metal-poor star forming regions. A description is given of the stellar data base used, including the effects of stellar mass loss and convective overshooting, the absorption features, and luminosity indicators. The gaseous emission component and synthesis method are discussed. Several models of the spectral evolution of the regions are calculated and compared with empirical data.

Affiliated with

Also associated with

No associations

Rating

Spectral evolutionary synthesis models of metal-poor star forming regions 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 Spectral evolutionary synthesis models of metal-poor star forming regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectral evolutionary synthesis models of metal-poor star forming regions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1612531