Title of article
26Al production in image Velorum Original Research Article
Author/Authors
N. Mowlavi، نويسنده , , J. Kn?dlseder، نويسنده , , G. Meynet، نويسنده , , P. Dubath، نويسنده , , R. Diehl، نويسنده , , G. Lichti، نويسنده , , S. Schanne، نويسنده , , C. Winkler، نويسنده ,
Issue Information
هفته نامه با شماره پیاپی سال 2005
Pages
4
From page
320
To page
323
Abstract
The closest Wolf-Rayet star, WR 11 in the binary system γ2 Velorum, is the only star for which the spectral signature of the 26Al produced in its core is expected to be detectable with current gamma-ray instruments, through the 1.8 MeV gamma-ray line produced by the radioactive decay of the 26Al nuclei.
We present here the current status of both model predictions, from calculations of massive star evolution including rotation of stellar interior, and from data on γ2 Velorum obtained by the ESAʹs gamma-ray satellite INTEGRAL over the first year of its mission.
Journal title
Nuclear physics A
Serial Year
2005
Journal title
Nuclear physics A
Record number
1202581
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