Gamma-Ray Line Emission from Superbubbles

Details Gamma-Ray Line Emission from Superbubbles Gamma-Ray Line Emission from Superbubbles

1999-03-11

arxiv.org/abs/astro-ph/9903170v1

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures, Proc. of the 3rd INTEGRAL workshop, Taormina

Scientific paper

We present an evolutionary model for gamma-ray line emission from superbubbles based on shock acceleration of metal-rich stellar ejecta. Application to the Orion OB1 association shows that gamma-ray lines at the detection threshold of the SPI spectrometer aboard of INTEGRAL are expected, making this region an interesting target for studies of the interaction of supernova shocks with the interstellar medium.

Affiliated with

Also associated with

No associations

Rating

Gamma-Ray Line Emission from Superbubbles does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Gamma-Ray Line Emission from Superbubbles, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gamma-Ray Line Emission from Superbubbles will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-266960