Multi-wavelength emission from massive star associations

Bibcode
2001ESASP.459...37C
Cerviño, M.; Knödlseder, J.; Schaerer, D.; von Ballmoos, P.; Meynet, G.
Referencia bibliográfica

In: Exploring the gamma-ray universe. Proceedings of the Fourth INTEGRAL Workshop, 4-8 September 2000, Alicante, Spain. Editor: B. Battrick, Scientific editors: A. Gimenez, V. Reglero & C. Winkler. ESA SP-459, Noordwijk: ESA Publications Division, ISBN 92-9092-677-5, 2001, p. 37 - 40

Fecha de publicación:
9
2001
Número de autores
5
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
Results from a new multi-wavelength evolutionary synthesis model including the γ-ray line emission from various radioactive isotopes (26Al, 60Fe) are presented. In particular the predicted γ-ray line observations combined with measurements of ionising fluxes can efficiently constrain the age of a stellar population, and help to identify the primary nucleosynthesis sources of the radioisotopes.
Tipo
Sin árbitro
Supernovas

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