Search for very high energy gamma-ray emission from parts of the Gould belt with the H.E.S.S. ground based Cherenkov telescopes
Files
(Published version)
Date
2007
Authors
Horns, D.
Rowell, G.
Aharonian, F.
Gabici, S.
Santangelo, A.
Schwarzburg, S.
Editors
Bellazzini, R.
Advisors
Journal Title
Journal ISSN
Volume Title
Type:
Conference paper
Citation
Proceedings of 30th International Cosmic Ray Conference (ICRC 2007), Merida, Yucatan, Mexico, 3-11 Jul 2007, Vol. 2 (OG part 1), pages 653–654
Statement of Responsibility
D. Horns, G.P. Rowell, F. Aharonian, S. Gabici, A. Santangelo, S. Schwarzburg for The H.E.S.S. Collaboration.
Conference Name
International Cosmic Ray Conference (30th : 2007 : Merida, Yucatan, Mexico)
Abstract
The Gould belt, a well-known region of enhanced star formation in the solar neighborhood, is observed to be an expanding rim with a diameter of a few hundred parsecs and a width of approximately 100 pc. Most of the nearby OB stellar associations and molecular clouds are found to be aligned with the Gould belt. With the high star formation rate along the Gould belt, the local supernova rate during the last few million years is believed to be three to four times larger than the Galactic average. Under the assumption that supernova remnants are efficient accelerators of cosmic rays, the Gould belt and its environment should show an increased cosmic ray density with respect to the Galactic average. The cosmic rays are expected to interact with the dense molecular gas which results mainly in pi-meson production with subsequent decay in gamma-rays and neutrinos. We have searched for gamma-ray emission from various nearby (d=100-200 pc) parts of the Gould belt with the HESS Cherenkov telescopes. Results will be presented at the conference.
School/Discipline
Dissertation Note
Provenance
Description
Access Status
Rights
© EDP Sciences. The original publication is available at www.edpsciences.org/alr.