γ-ray line emissions as tracers of tenuous phases of the interstellar medium

Details γ-ray line emissions as tracers of tenuous phases of the interstellar medium γ-ray line emissions as tracers of tenuous phases of the interstellar medium

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aipc..170..194h&link_type=abstract

AIP Conference Proceedings, Volume 170, pp. 194-195 (1988).

Computer Science

Scientific paper

γ-ray line emissions, produced by e+ annihilations and the decay
of 26Al, provide unique tools for probing on galactic scale the tenuous
interstellar phase-the least understood component of the interstellar
medium.

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