Detection of high-velocity 26AI towards the Galactic Centre
Detection of high-velocity 26AI towards the Galactic Centre
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Publisher
London: Nature Publishing Group UK
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Language
English
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London: Nature Publishing Group UK
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Contents
THEORY predicts
1
that radioactive
26
A1 (which has a half-life of 0.72 Myr) is released into the interstellar medium by nova and supernova explosions, from the winds of massive stars in the Wolf–Rayet phase, and from less-massive giant stars in very late stages of the asymptotic giant branch phase. Observations of 1,809-keV γ-ray emiss...
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Full title
Detection of high-velocity 26AI towards the Galactic Centre
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TN_cdi_proquest_miscellaneous_743182561
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_743182561
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ISSN
0028-0836
E-ISSN
1476-4687
DOI
10.1038/384044a0
