The synthesis of Al-26 in massive stars

Details The synthesis of Al-26 in massive stars The synthesis of Al-26 in massive stars

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...218..123w&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 218, no. 1-2, July 1989, p. 123-130.

Astronomy and Astrophysics

Astrophysics

17

Aluminum 26, Blue Stars, Gamma Ray Astronomy, Nuclear Astrophysics, Abundance, Stellar Composition

Scientific paper

After the discovery of the 1.8 MeV interstellar gamma-ray line associated with the beta-disintegration of Al-26, several processes were proposed to explain the aluminum synthesis. At the present time, massive stars seem to be a greater producer of Al-26 production rate for massive stars is very sensitive to convection and mass loss rate. The contribution of massive stars with a moderate overshooting and of the ON blue stragglers, which are considered to evolve homogeneously (Maeder, 1987) is estimated.

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