No CrossRef data available.
Article contents
Gamma-Ray Line Spectroscopy Results from COMPTEL
Published online by Cambridge University Press: 25 May 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
Comptel aboard NASA's Compton Observatory has led to a major progress in the field of astronomical gamma-ray line spectroscopy. Highlights are the all-sky map of the 1.8 MeV line from radioactive 26Al, the first detection of the 1.156 MeV line from radioactive 44Ti from a Supernova remnant (Cas A), and the detection of excessive MeV emission from the Orion complex that may be ascribed to excitation of 12C and 16O nuclei.
- Type
- Session 1: Plasma and Fresh Nucleosynthesis Phenomena
- Information
- Copyright
- Copyright © Kluwer 1998
References
3.
Oberlack, U., 1997, :
Über die Natur der Galaktischen 26Al Quellen: Untersuchung des 1.8 MeV Himmels mit COMPTEL
,
Google Scholar
5.
Hartmann, D. et al., 1997, Proc. of 4th Int. Conf. on Nucl. in the Cosmos Notre Dame, USA, Nucl. Phys. A.
Google Scholar
8.
Parizot, E.M.G., 1997, submitted to A&A, and Proc. of 4th Compton Symp., AIP, in press
Google Scholar
You have
Access