Operational Health Physics Training by HJ Moe
Electromagnetic form factors in the relativized Hypercentral CQM E. Santopinto Trieste 22_26 May 2006 M. Ferraris, M.Giannini, M. Pizzo, E. Santopinto,
How Do Particle Accelerators Work?. If you have an older tv, you own an accelerator! Acceleration occurs when a charged particle falls through a voltage.
Polarization in Pulsar Wind Nebulae Delia Volpi In collaboration with: L. Del Zanna - E. Amato - N. Bucciantini Dipartimento di Astronomia e Scienza dello.
Fluorescence – a key to unravel (atomic) structure and dynamics.
Backreaction as an explanation for Dark Energy ? with some remarks on cosmological perturbation theory James M. Bardeen University of Washington The Very.
Dalton 2015 Manual
June 26, 2009 64 th International Symposium on Molecular Spectroscopy The Pure Rotational Spectrum of ZnS (X 1 + ) Lindsay N. Zack Lucy M. Ziurys Department.
Hyperfine-Changing Collisions of Cold Molecules J. Aldegunde, Piotr Żuchowski and Jeremy M. Hutson University of Durham EuroQUAM meeting Durham 18th April.
The high mass accretion rate spectra of GX 339-4: Black hole spin from reflection? Mari Kolehmainen & Chris Done, Durham University Maria Diaz Trigo, ESO.
Session: MGAT9 – Self-Gravitating Systems SPHERICALLY SYMMETRIC RELATIVISTIC STELLAR CLUSTERS WITH ANISOTROPIC MOMENTUM DISTRIBUTION Marco MERAFINA Department.
High-Precision Sub-Doppler Infrared Spectroscopy of HeH + Adam J. Perry, James N. Hodges, Charles Markus, G. Stephen Kocheril, Paul A. Jenkins II, and.
