Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011hsa6.conf..518z&link_type=abstract
Highlights of Spanish Astrophysics VI, Proceedings of the IX Scientific Meeting of the Spanish Astronomical Society (SEA), held
Astronomy and Astrophysics
Astrophysics
Scientific paper
The MAGIC collaboration has recently reported correlated X-ray and VHE gamma-ray emission from the gamma-ray binary during about 60% of one orbit, thus suggesting that the emission in these two bands has its origin in a single particle population. Using a one zone population of relativistic leptonic particles with dominant adiabatic losses located at the position of the compact object we are able to reproduce the observed X-ray and VHE lightcurves. From the best fit result, we obtain the magnetic field, energy budget and acceleration efficiency of the accelerator, and discuss these in the context of the young non-acretting pulsar and acretting compact object scenarios. The results also confirm that the GeV emission detected by Fermi does not come from the same parent particle population as the X-ray and VHE emission.
Bosch-Ramon Valenti
Paredes Javier M.
Zabalza Victor
No associations
LandOfFree
A leptonic one-zone model of the X-Ray/VHE correlated emission in LS I +61 303 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A leptonic one-zone model of the X-Ray/VHE correlated emission in LS I +61 303, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A leptonic one-zone model of the X-Ray/VHE correlated emission in LS I +61 303 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-740807