HESS observations of the Carina nebula and its enigmatic colliding wind binary Eta Carinae
Abstract
The massive binary system Eta Carinae and the surrounding H II complex, the Carina nebula, are potential particle acceleration sites from which very high energy (VHE; E≥ 100 GeV) γ-ray emission could be expected. This paper presents data collected during VHE γ-ray observations with the HESS telescope array from 2004 to 2010, which cover a full orbit of Eta Carinae. In the 33.1-h data set no hint of significant γ-ray emission from Eta Carinae has been found and an upper limit on the γ-ray flux of ? (99 per cent confidence level) is derived above the energy threshold of 470 GeV. Together with the detection of high energy (HE; 0.1 ≤E≤ 100 GeV) γ-ray emission by the Fermi Large Area Telescope up to 100 GeV, and assuming a continuation of the average HE spectral index into the VHE domain, these results imply a cut-off in the γ-ray spectrum between the HE and VHE γ-ray range. This could be caused either by a cut-off in the accelerated particle distribution or by severe γ-γ absorption losses in the wind collision region. Furthermore, the search for extended γ-ray emission from the Carina nebula resulted in an upper limit on the γ-ray flux of ? (99 per cent confidence level). The derived upper limit of ∼23 on the cosmic ray enhancement factor is compared with results found for the old-age mixed-morphology supernova remnant W28.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- July 2012
- DOI:
- 10.1111/j.1365-2966.2012.21180.x
- arXiv:
- arXiv:1204.5690
- Bibcode:
- 2012MNRAS.424..128H
- Keywords:
-
- acceleration of particles;
- radiation mechanisms: non-thermal;
- ISM: individual objects: Carina nebula;
- ISM: individual objects: Eta Carina;
- open clusters and associations: general;
- X-rays: binaries;
- Astrophysics - High Energy Astrophysical Phenomena;
- Astrophysics - Astrophysics of Galaxies
- E-Print:
- 8 pages, 3 figures, accepted for publication in MNRAS