Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/37506
Citations | ||
Scopus | Web of Science® | Altmetric |
---|---|---|
?
|
?
|
Type: | Journal article |
Title: | Discovery of the two 'wings' of the Kookaburra complex in VHE γ-rays with HESS |
Other Titles: | Discovery of the two 'wings' of the Kookaburra complex in VHE gamma-rays with HESS |
Author: | Aharonian, F. Akhperjanian, A. Bazer-Bachi, A. Beilicke, M. Benbow, W. Berge, D. Bernlohr, K. Boisson, C. Bolz, O. Borrel, V. Braun, I. Brown, A. Buhler, R. Busching, I. Carrigan, S. Chadwick, P. Chounet, L. Cornils, R. Costamante, L. Degrange, B. et al. |
Citation: | Astronomy and Astrophysics: a European journal, 2006; 456(1):245-251 |
Publisher: | E D P Sciences |
Issue Date: | 2006 |
ISSN: | 0004-6361 1432-0746 |
Statement of Responsibility: | F.Aharonian ... G.Rowell ... M.Ward ... et al. |
Abstract: | Aims. Search for Very High Energy γ-ray emission in the Kookaburra complex through observations with the HESS array. Methods. Stereoscopic imaging of Cherenkov light emission of the γ-ray showers in the atmosphere is used for the reconstruction and selection of the events to search for γ-ray signals. Their spectrum is derived by a forward-folding maximum likelihood fit. Results. Two extended γ-ray sources with an angular (68%) radius of 3.3-3.4′ are discovered at high (>13σ) statistical significance: HESS J1420-607 and HESS J1418-609. They exhibit a flux above 1 TeV of (2.97 ±0.188stat ±0.60sys) × 1012 and (2.17 ±0.17stat ±0.43sys) × 1012 cm-2 s-1, respectively, and similar hard photon indices ∼2.2. Multi-wavelength comparisons show spatial coincidence with the wings of the Kookaburra. Two pulsar wind nebulae candidates, K3/PSR J1420-6048 and the Rabbit, lie on the edge of the HESS sources. Conclusions. The two new sources confirm the non-thermal nature of at least parts of the two radio wings which overlap with the γ-ray emission and establish their connection with the two X-ray pulsar wind nebulae candidates. Given the large point spread function of EGRET, the unidentified source(s) 3EG J1420-6038/GeV J1417-6100 could possibly be related to either or both HESS sources. The most likely explanation for the Very High Energy γ-rays discovered by HESS is inverse Compton emission of accelerated electrons on the Cosmic Microwave Background near the two candidate pulsar wind nebulæ, K3/PSR J1420-6048 and the Rabbit. Two scenarios which could lead to the observed large (∼10 pc) offset-nebula type morphologies are briefly discussed. © ESO 2006. |
Rights: | © The European Southern Observatory 2006 |
DOI: | 10.1051/0004-6361:20065511 |
Published version: | http://dx.doi.org/10.1051/0004-6361:20065511 |
Appears in Collections: | Aurora harvest 6 Physics publications |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
hdl_37506.pdf | Published version | 855.7 kB | Adobe PDF | View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.