Affiliation
The University of Adelaide
Main category
Natural Sciences (Astrophysics and Astrononmy)
Abstract
The HESS sources HESS J1614-518 and HESS J1616-508 have yet to be associated with any potential accelerator such as supernova remnants, pulsar wind nebulae, Wolf-Rayet stars or stellar clusters. We use the recently available Mopra CO survey to conduct a first look study into the molecular gas towards the HESS sources to attempt to understand the hardonic situation.
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