English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Journal Article

ISM Studies Towards Several PWNe

MPS-Authors
/persons/resource/persons30244

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

External Resource
No external resources are shared
Fulltext (restricted access)
There are currently no full texts shared for your IP range.
Fulltext (public)
There are no public fulltexts stored in PuRe
Supplementary Material (public)
There is no public supplementary material available
Citation

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
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 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.