[W24] Emmanuel Moulin: The inner 300 parsec of the Galactic Centre seen by H.E.S.S.

Wednesday 15 June 2016, 15.00 UTC

Q&A at google+

The inner 300 parsec of the Galactic Centre seen by H.E.S.S.

Speaker: Emmanuel Moulin, CEA-Saclay.

Host: Alejandro de La Puente, Carleton U.

The Galactic Centre region has been observed by the High Energy Stereoscopic System (H.E.S.S.) array of ground-based Cherenkov telescopes since 2004 leading to the detection of the very-high-energy (VHE, E > 100 GeV) gamma-ray source HESS J1745−290 spatially coincident with the supermassive black hole Sgr A*. Diffuse TeV gamma-ray emission has been detected along the Galactic plane, most likely due to cosmic-ray interactions with the dense gas of the Central Molecular Zone. The rich 2004-2013 dataset allows for detailed spectral and morphological studies the inner 200 pc of the Galactic Centre region. The new results allow us to make an important statement regarding the location and origin of the accelerator of the parent ultrarelativistic particles. I will discuss the H.E.S.S. observations of the Galactic Centre region in the context of the origin of Galactic cosmic rays.

Leave a Reply

Please log in using one of these methods to post your comment:

WordPress.com Logo

You are commenting using your WordPress.com account. Log Out /  Change )

Google photo

You are commenting using your Google account. Log Out /  Change )

Twitter picture

You are commenting using your Twitter account. Log Out /  Change )

Facebook photo

You are commenting using your Facebook account. Log Out /  Change )

Connecting to %s

This site uses Akismet to reduce spam. Learn how your comment data is processed.