newtonian and non newtonian behaviour of fluids
Nguyen 2015
1-s2.0-S0093641303000673-main
Collaborators: Wong A. Y. L. (HKU), Huang, Y. F. (NJU), Cheng, K. S. (HKU), Lu T. (PMO), Xu M. (NJU), Wang X. (NJU), Deng W. (NJU). Gamma-ray Sky from.
K.J. Shah Physical Research Laboratory (Unit of Dept. of Space, Govt. of India) Navrangpura, Ahmedabad – 380 009.
The Ultra-luminous X-Ray Sources Near the Center of M82 NTHU 10/18/2007 Yi-Jung Yang.
Comoving Acceleration by Relativistic Poynting Flux Edison Liang Rice University Acknowledgements: Kasumi Nishimura, Koichi Noguchi (Japan); Peter Gary,
The Ultra-luminous X-Ray Sources Near the Center of M82
Temporal evolution of thermal emission in GRBs
Particle Acceleration and Radiation from Poynting Jets and Collisionless Shocks Edison Liang, Koichi Noguchi Rice University Acknowledgements: Scott Wilks,
Locarno, 8 June 2005Peter Gallagher (UCD) Chromospheric Evaporation Peter Gallagher University College Dublin Ryan Milligan Queens University Belfast.
What the UV SED Can Tell Us About Primitive Galaxies
