Fluorescence and resonant ionization in astrophysical plasmas, with emphasis on and examples from the star Eta Carinae
Science paper H
Sambit-presentation
SUPERNOVAE The Brightest Lights in the Universe By Michael Davis.
On the Main Sequence What holds a star up while it is on the MS? Parts of a MS star How does energy get out? Radiation & Convection May take a million.
The Bohr Model and the Quantum Mechanical Model of the Atom Physics 12.
Precision test of bound-state QED and the fine structure constant Savely G Karshenboim D.I. Mendeleev Institute for Metrology (St. Petersburg) and Max-Planck-Institut.
Applications of Iceland spar prisms in observational astronomy, 1860-1930 Leó Kristjánsson Institute of Earth Sciences.
Gamma-ray bursts Discovered in 1968 by Vela spy satellites Occur ~ 3 times a day at random positions in the sky.
Astronomy Temperature, Luminosity, & H-R Diagram.
The Sun
Hydrogen Lines in DA White Dwarfs: Improved Stark Broadening
