A brief review is presented of the major targets for gamma-ray spectroscopy of supernovae. The chief utility of such observations is the new insight they provide into the mechanisms of supernova explosions, the distribution and nature of star forming regions in our Galaxy, and our Galaxy's nucleosynthetic history. The discussion centers on two short lived species, 56Co and 44Ti, which might be seen in individual events, and two longer lived species, 26Al and 60Fe, which are the generally seen as the cumulative production of many supernovae.
|Original language||English (US)|
|Title of host publication||European Space Agency, (Special Publication) ESA SP|
|Number of pages||4|
|State||Published - 1997|
- Nucleosynthesis, gamma-line spectroscopy
ASJC Scopus subject areas
- Aerospace Engineering