Linje shape diagnostics of galactic 26Al

Details Linje shape diagnostics of galactic 26Al Linje shape diagnostics of galactic 26Al

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...20311208h&link_type=abstract

American Astronomical Society Meeting 203, #112.08; Bulletin of the American Astronomical Society, Vol. 35, p.1385

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Scientific paper

The production of radioactive 26Al in supernovae, and other sources, provides a unique tracer of the global galactic star formation history. The 1.8 MeV line resulting from the decay of 26Al has been detected and mapped. The line shape is affected by the kinematic properties of these nuclei, resulting from the ejection dynamics and galactic differential rotation. We discuss the line observations at 1.8 MeV and their theoretical interpretation.

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