Freiburg 2008 – wissenschaftliches Programm
Bereiche | Tage | Auswahl | Suche | Downloads | Hilfe
EP: Fachverband Extraterrestrische Physik
EP 15: Astrophysics III
EP 15.1: Vortrag
Donnerstag, 6. März 2008, 14:00–14:15, KGI-Aula
MAGIC Telescope observations of high energy gamma-rays from globular cluster M13 — •Julian Sitarek1,2, Tobias Jogler1, and Wlodek Bednarek2 for the MAGIC collaboration — 1Max-Planck-Institut für Physik, München, Germany — 2Division of Experimental Physics, University of Lodz, Lodz, Poland
Globular clusters are quite compact (size ∼ 10 pc) objects distributed spherically around the galaxy. They contain about 105 - 106 mostly old stars. The number of milisecond pulsars in typical globular cluster is expected to be large (of the order of 100). We investigate the possible mechanism of production of high energy gamma-rays in those objects. Part of the wind energy of pulsars (energy conversion factor) is converted into relativistic leptons. Those leptons can upscatter in inverse Compton process low energy starlight and CMB photons and produce gamma-rays.
MAGIC is an Imaging Atmospheric Cerenkov Telescopes located at Canary island of La Palma. We present results and discussion of the MAGIC observations of globular cluster M13.