Stellar collision

Related lectures (25)

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Explores physical concepts in astrophysics to understand light radiation from celestial bodies.

Covers stellar evolution, fusion processes, and the age of stellar clusters, emphasizing gas pressures and star evolution based on mass.

Explores the formation and evolution of galaxies, galactic dynamics, stellar orbits, and equilibria of collisionless systems in astrophysics.

Covers astronomical units, light years, parallax, exoplanets, stars, nebulae, and galaxy clusters.

Explores the conditions for gravitational collapse and the life time of stars through fusion processes.

Covers dark matter detection challenges and the evolution of massive stars into neutron stars.

Explores Primordial Black Holes, their formation, gravitational wave signatures, constraints on abundance, and future detection prospects.

Introduces the course on Stellar and Galactic Dynamics, covering self-gravitating systems and their evolution under gravity.

Explores the measurement of the Hubble Constant using gravitational waves and the standard siren method.

Delves into the stability of stellar systems through perturbation and linear response theories, including the Jeans instability.