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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 |
Appears in Collections: | Aurora harvest 8 Physics publications |
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