Speakers
Description
Peter Marinos aims to simulate the Galactic TeV diffuse gamma-ray emission with GALPROP for a variety of model parameters, and to make comparisons between these models and the diffuse emission estimated by the H.E.S.S. telescope array in their Galactic plane survey.
Kirsty Feijen aims to reveal the origin of HESS J1804−216 by modelling both the spectral and spatial gamma-ray morphology from SNRs in the hadronic scenario.
Adnaan Thakur: SNR RXJ1713.7-3946 is a one of the brightest young supernova remnants detected by the HESS Galactic Plane Survey. We have studied the C[II], HI and H_2 emission from the region and will provide an update on our analysis.
Rami Alsulami: I investigate the optical outflow towards the Scutum Supershell using multi-wavelength observations (X-rays, TeV gamma rays and optical H alpha. I also investigate possible scenarios for the origin of such an extended outflow.
