1. ISM Studies Towards Several PWNe.
- Author
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Voisin, F., Rowell, G., Burton, M. G., Fukui, Y., Sano, H., and Aharonian, F.
- Subjects
- *
GAMMA ray astronomy , *INTERSTELLAR medium , *PULSARS , *NEBULAE , *ASTRONOMICAL observations - 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. [ABSTRACT FROM AUTHOR]
- Published
- 2017
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