Stellar Astronomy
Stars: their formation, structure, evolution, and endpoints.
Articles (4)
- White Dwarfs
The dense, cooling remnants of Sun-like stars supported by electron degeneracy pressure, with a maximum mass of about 1.4 solar masses. - Black Holes
Regions of spacetime where gravity is so strong that nothing, not even light, can escape from inside the event horizon. - Stellar Nucleosynthesis
How stars build chemical elements from hydrogen through nuclear fusion, and how explosions and stellar winds spread them into space. - Neutron Stars
Ultra-dense stellar remnants formed in supernovae: their structure, the pulsar mechanism, and what their mergers teach about matter and elements.