The Impact of Magnetic Stresses and Inhomogeneities on Accretion Disk Spectra
Baryonic Dark Matter and Galaxy Formation
Lecture 10 : Statistical thermal model Hadron multiplicities and their correlations and fluctuations (event-by-event) are observables which can provide.
Non-Local Thermodynamic Equilibrium
Lecture 10 : Statistical thermal model
The Economics of Equity: Insights from Econophysics and the BDY Model By: G.H. Boyle 2 nd Oct CANUSSEE 2015 Screen shot from EiLab – at orrery-software.webs.com.
Signatures of stellar surface structure Dainis Dravins - Lund Observatory
The transition to strong convection
Tropical Cyclone Intrinsic Variability & Predictability
Understanding the Properties of Chemical Freeze-Out
