Mopra and Nanten Studies of HESS J1825-137 Northern Cloud

Voisin, F.; Rowell, G.; Fukui, Y.; Burton, M.; Walsh, A.; Aharonian, Felix A.

doi:10.1142/S2010194514601999

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Mopra and Nanten Studies of HESS J1825-137 Northern Cloud

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

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Citation

Voisin, F., Rowell, G., Fukui, Y., Burton, M., Walsh, A., & Aharonian, F. A. (2014). Mopra and Nanten Studies of HESS J1825-137 Northern Cloud. International Journal of Modern Physics: Conference Series, 28: 1460199. doi:10.1142/S2010194514601999.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0019-029F-3

Abstract

The Pulsar Wind Nebula (PWN) HESS J1825-137 is one of the most extended TeV PWN and its morphology is influenced by the molecular gas located north of the TeV sources. In order to refine the composition and dynamics of the cloud, we have used the telescope Mopra in the 7 and 12 mm bands. Our results highlight dense regions and also perturbations in the southern part of the dense cloud.