Chapter 13 Cont’d – Pressure Effects More curves of growth How does the COG depend on excitation potential, ionization potential, atmospheric parameters.
Hydrogen Lines in DA White Dwarfs: Improved Stark Broadening
Non-Local Thermodynamic Equilibrium
Conclusions The prototype Pup (O4 I) has X-ray emission line profiles consistent with a simple spherically symmetric wind shock model. What can lead.
Abundances in the solar system: what we achieved and how much was it dependent on space probes?
Conclusions
