Evolutionary synthesis models for the emission from radioactive isotopes in H ii regions

Details Evolutionary synthesis models for the emission from radioactive isotopes in H ii regions Evolutionary synthesis models for the emission from radioactive isotopes in H ii regions

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000newar..44..321c&link_type=abstract

New Astronomy Reviews, Volume 44, Issue 4-6, p. 321-327.

Astronomy and Astrophysics

Astronomy

Scientific paper

We have extended our evolutionary synthesis models for Star Forming Regions to the /γ-ray domain. Applying different yields to the resulting synthetic populations, we obtain lightcurves of γ-ray line emission due to the radioactive decay of stellar nucleosynthesis products, such as 26Al and 60Fe. We present here this time evolution and the application of the models to regions of star formation in our galaxy.

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