Expert-level astrophysics covering stellar physics, galaxy formation, high-energy astrophysics, observational techniques, and the electromagnetic spectrum across wavelengths.
Stellar structure: hydrostatic equilibrium, energy transport by radiation and convection. Nuclear burning: pp chain and CNO cycle produce energy in stellar cores. HR diagram: luminosity vs temperature, main sequence, giants, white dwarfs. Stellar evolution: main sequence to red giant to white dwarf or supernova. Stellar remnants: white dwarf, neutron star, black hole depending on mass.
Galaxy types: elliptical, spiral, irregular, lenticular. Dark matter halo: dominates mass, traced by rotation curves and lensing. Star formation: molecular clouds, Jeans criterion, feedback processes. AGN: active galactic nuclei, supermassive black hole accretion. Galaxy mergers: major and minor mergers, morphological transformation.
X-ray binaries: neutron star or black hole accreting from companion. Gamma-ray bursts: most energetic explosions, short from mergers and long from collapsars. Supernovae: Type Ia thermonuclear and Type II core collapse, distance indicators. Cosmic rays: high-energy particles, sources include SNR and AGN jets.
Photometry: measuring flux in broadband filters, magnitudes and colors. Spectroscopy: resolving spectral features, redshift, chemical abundances. Interferometry: combining multiple telescopes for higher angular resolution. Gravitational waves: LIGO and Virgo detect mergers of compact objects.
| Pitfall | Fix |
|---|---|
| Ignoring dust extinction | Apply reddening correction in optical and NIR |
| Confusing luminosity and flux | Convert to intrinsic luminosity using distance |
| Wrong cosmology for distance | Specify H0 and cosmological parameters used |
| Selection bias in samples | Characterize selection function of survey |