Philips Atlas of the Universe
Asymptotic Giant Branch. Learning outcomes Evolution and internal structure of low mass stars from the core He burning phase to the tip of the AGB Nucleosynthesis.
Red Giant Phase to Remnant (Chapter 10). Student Learning Objective Describe or diagram the evolutionary phases from the beginning of stellar formation.
Transit Timing Variations
General Astronomy
Chapter 17: Evolution of High-Mass Stars. Massive stars have more hydrogen to start with but they burn it at a prodigious rate The overall reaction is.
