The Gas Survey of HESS J1614-518 and HESS J1616-508 using the Mopra Telescope
1085 views
11.12.2015
Co-author
Gavin Rowell
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.
Further information
Further reading
Language
DOI
Conference
Do you have problems viewing the pdf-file? Download presentation here
If the presentation contains inappropriate content, please report the presentation. You will be redirected to the landing page.