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

Bibcode
2000NewAR..44..321C
DOI
10.1016/S1387-6473(00)00034-8
Cerviño, M.; Knödlseder, Jürgen; Schaerer, Daniel; von Ballmoos, Peter
Referencia bibliográfica

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

Fecha de publicación:
7
2000
Revista
New Astronomy Reviews
Número de autores
4
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
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.
Tipo
Con árbitro

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