Stability of Rotating Systems

Related lectures (32)

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

Explores the Milky Way's structure and galaxy classification based on the Hubble-De Vaucouleurs Sequence.

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

Covers the Milky Way, galaxy classification, types, and structures.

Explores galaxy formation, debunking misconceptions and showcasing digital simulations of spiral galaxies evolving into elliptical galaxies.

Explores the stability of rotating systems, focusing on spiral structures and the winding problem in observed spirals.

Explores dark matter in galaxies and clusters, rotation curves, and the m / l ratio.

Delves into the nature and properties of the first stars, exploring galaxy evolution and nucleosynthesis signatures.

Covers the hot big bang theory, its origins, and implications for cosmology.

Explores the contents and properties of the observable universe, including galaxy sizes, mass, and morphologies.