AST 5.2 PPT
The Secondary Stars of Cataclysmic Variables Christian Knigge arXiv:1101.1538v2 reporter:ShaoYong.
An Astronomy GradNet Tech Talk: Searching for Eclipsing Binary Stars Jonathan Devor, Ph.D. October 20, 2008.
Neutron Star Formation and the Supernova Engine Bounce Masses Mass at Explosion Fallback.
Neutrinos from Stellar Collapse Chris Fryer (LANL/UNM) “Normal” Core Collapse: Collapse and Bounce, Fallback and Cooling More massive Stars Low Mass Stars.
The Formation and Structure of Stars Chapter 9. Stellar Models The structure and evolution of a star is determined by the laws of: Hydrostatic equilibrium.
Exploding stars And the modeling of Dwarf galaxies .
A new approach to the 176 Lu puzzle clock or thermometer? an astrophysical quest and a nuclear challenge 20 years of nuclear physics level schemes,
Stellar Evolution. The Life of a Star Mass Is the Key Stars require millions to billions of years to evolve – a time that is incredibly slow by human.
Chapter 13 Stellar Evolution Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
White Dwarfs. References D. Koester, A&A Review (2002) “White Dwarfs: Recent Developments” Hansen & Liebert, Ann Rev A&A (2003) “Cool White Dwarfs” Wesemael.
APOGEE: The Apache Point Observatory Galactic Evolution Experiment l M. P. Ruffoni 1, J. C. Pickering 1, E. Den Hartog 2, G. Nave 3, J. Lawler 2, C. Allende-Prieto.
