Atomic physics of shocked plasma in the winds of massive stars
European Space Astronomy Centre Villafranca del Castillo, Madrid, Spain Andy Pollock XMM-Newton SOC High-Resolution X-rays from Hot Stars Physics and Dynamics.
12 Years of ChandraMay 23, 2011 X-ray Line Diagnostics of Shocked Outflows in Eta Carinae and Other Massive Stars M. F. Corcoran.
A Survey of Local Group Galaxies Currently Forming Stars Phil Massey Lowell Observatory April 14, 2003.
Evolutionary Population Synthesis models Divakara Mayya INAOEydm Advanced Lectures on Galaxies (2008 INAOE): Chapter 4.
Are Stellar Eruptions a Common Trait of SNe IIn? Baltimore, MD 06/29/11 Ori Fox NPP Fellow NASA Goddard Based on arXiv:1104.5012.
A Survey of Local Group Galaxies Currently Forming Stars
Discordant Estimates of Mass-Loss Rates for O-Type Stars
Evolutionary Population Synthesis models
X-ray Line Profile Diagnostics of Shock Heated Stellar Winds
X-ray Line Diagnostics of Shocked Outflows in Eta Carinae and Other Massive Stars
