Stellar Astronomy and Astrophysics
Stellar Astronomy and Astrophysics is the branch of astrophysics dedicated to the study of stars, encompassing their entire life cycle from birth in interstellar gas clouds to their eventual demise as remnants like white dwarfs, neutron stars, or black holes. By applying the principles of physics—particularly nuclear physics, thermodynamics, and radiative transfer—to observational data, this field seeks to understand the internal structure, atmospheric properties, energy generation, and chemical evolution of stars. This knowledge is fundamental not only for understanding individual celestial objects but also for deciphering the larger-scale evolution of galaxies and the synthesis of chemical elements throughout the cosmos.
- Introduction to Stellar Astrophysics
- Fundamental Concepts and Scales
- Foundational Physics
- Observational Tools and Techniques
- Telescopes and Instrumentation
- Photometry
- Spectroscopy
- Astrometry
- Interferometry