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Journal Article

ISM Studies Towards Several PWNe


Aharonian,  F. A.
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Voisin, F., Rowell, G., Burton, M. G., Fukui, Y., Sano, H., & Aharonian, F. A. (2017). ISM Studies Towards Several PWNe. AIP Conference Proceedings, 1792: 040011. doi:10.1063/1.4968915.

Cite as: https://hdl.handle.net/21.11116/0000-0000-BB08-5
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 III 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.