Rino Bandiera, OAAFundamental Physics & Astrophysics of SNRsSNA07, May 20-26, 2007 Fund. Physics & Astrophysics of Supernova Remnants Lecture #1 –What.
1 Using JAXA's Space Science Data for Education and Public Outreach JAXA/ISAS PLAIN center Ken EBISAWA.
Simulated synchrotron emission from Pulsar Wind Nebulae Delia Volpi Dipartimento di Astronomia e Scienza dello Spazio-Università degli Studi di Firenze-Italia.
Neutron Star Powered Nebulae
LIGO Magazine Issue 1
TeV Observations of the Galactic Plane with HAWC and Joint Analysis of GeV Data from Fermi
2009 July 8 Supernova Remants and Pulsar Wind Nebulae in the Chandra Era 1 Modeling the Dynamical and Radiative Evolution of a Pulsar Wind Nebula inside.
Neutron Star Environment: from Supernova Remnants to Pulsar Wind Nebulae Stephen C.-Y. Ng McGill University Special thanks to Pat Slane for some materials.
KM3NeT: The Future km 3 -Scale Telescope in the Mediterranean Sea Scientific motivation Current Projects: ANTARES, NEMO, NESTOR The KM3NeT Design.
Particle acceleration in Pulsar Wind Nebulae Elena Amato INAF-Osservatorio Astrofisico di Arcetri Collaborators: Jonathan Arons, Niccolo’ Bucciantini,Luca.
KM3NeT: Towards a km 3 Mediterranean Neutrino Telescope Some Physics Arguments Aiming at a km 3 Detector in the Mediterranean Sea The KM3NeT Design.
The KM3NeT Project: A km 3 –Scale Mediterranean Neutrino Telescope and Deep-Sea Research Infrastructure Scientific Case Technical Aspects The KM3NeT.
