Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/105756
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Type: Conference paper
Title: ISM studies towards several PWNe
Author: Voisin, F.
Rowell, G.
Burton, M.
Fukui, Y.
Sano, H.
Aharonian, F.
Citation: AIP Conference Proceedings, 2017 / Aharonian, F., Hofmann, W., Rieger, F. (ed./s), vol.1792, pp.040011-1-040011-6
Publisher: American Institute of Physics
Issue Date: 2017
Series/Report no.: AIP Conference Proceedings
ISBN: 9780735414563
ISSN: 0094-243X
1551-7616
Conference Name: 6th International Meeting on High Energy Gamma-Ray Astronomy (11 Jul 2016 - 15 Jul 2016 : Heidelberg, Germany)
Editor: Aharonian, F.
Hofmann, W.
Rieger, F.
Statement of
Responsibility: 
F. Voisin, G. Rowell, M. G. Burton, Y. Fukui, H. Sano and F. Aharonian
Abstract: Pulsar wind Nebulae (PWNe) represent the largest population of TeV sources detected by H.E.S.S. Here, we present a ISM study combining 7mm Mopra observations with Nanten CO(1–0) and SGPS Hi data to understand the ISM environment towards HESS J1809−193, HESS J1026−582 and HESS J1826−130, as well as the morphology of the TeV source gamma-ray emission. Combining the TeV emission with several extended dense regions will then be useful to quantify the distinguish the contribution from PWNe and SNRs towards various HESS TeV sources.
Rights: © The author. © AIP Publishing LLC Proceedings issue.
DOI: 10.1063/1.4968915
Published version: http://dx.doi.org/10.1063/1.4968915
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