Speaker
Sunanda .
Description
TXS0506+056 is the first-ever known blazar having ∼3.5σ spatial and temporal correlation with IceCube neutrino alert 170922A, this source has been observed in multi-wavelengths during different epochs. A multi-wavelength study of this source during different epochs suggests a time delay between high and Very high energy gamma(VHE) emission. Here, we propose this time delay could be explained by two interaction channels electron synchrotron, SSC and proton synchrotron.
| Session | Astroparticle Physics and Cosmology |
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Author
Co-author
Dr
Reetanjali Moharana
(Indian Institute of Technology Jodhpur, Rajasthan India)
