Prospects for observing supernova products from Cas A and the Vela region with SPI

Details Prospects for observing supernova products from Cas A and the Vela region with SPI Prospects for observing supernova products from Cas A and the Vela region with SPI

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.459...97s&link_type=abstract

In: Exploring the gamma-ray universe. Proceedings of the Fourth INTEGRAL Workshop, 4-8 September 2000, Alicante, Spain. Editor:

Physics

Gamma Rays, Supernova Remnants, Nucleosynthesis, Integral Spectrometer

Scientific paper

The study of gamma-ray line afterglows from supernova radioactivities is a major objective for the SPI Spectrometer on INTEGRAL. The decay lines of 44Ti and 26Al are the main candidates. We discuss prospects for observing two SNR with observation times similar to those available in the core program. Since the lines are expected to be Doppler broadened, we study the effect of line-width on the detectability of SNR.

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