Galaxy Formation: Digital Illustrations

In course

Mollit labore ad sunt quis eiusmod qui. Aliqua magna incididunt duis incididunt eiusmod esse. Commodo eiusmod eu incididunt qui fugiat aliqua est in cillum enim esse ipsum. Mollit esse elit duis aute ut anim excepteur eiusmod proident commodo sunt. Id nostrud velit do aliquip fugiat incididunt Lorem Lorem labore do et aliqua culpa proident.

Description

This lecture explores the various formation modes of galaxies, debunking the misconception that elliptical galaxies evolve into spiral galaxies. It delves into the role of collisions between galaxies, the influence of dark matter, and kinetic properties on galaxy formation. The simulation presented demonstrates the collapse of matter, the formation of structures like spiral galaxies, and their eventual destruction in galaxy clusters. It also showcases extreme cases of galaxy interactions resulting in the transformation of spiral galaxies into compact elliptical galaxies.

In MOOCs (3)

Instructor

voluptate nisi elit

Proident duis aliquip enim ullamco cillum excepteur dolore proident ad eu proident deserunt. Ipsum irure quis enim labore ex voluptate pariatur sit. Minim occaecat et voluptate tempor et esse laboris eu occaecat fugiat esse est excepteur. Aute consectetur aliqua eiusmod velit. Dolor consequat ad cupidatat aute reprehenderit excepteur magna ad Lorem irure in.

Official source

https://mediaspace.epfl.ch/media/0_g65vwo0x

About this result

This page is automatically generated and may contain information that is not correct, complete, up-to-date, or relevant to your search query. The same applies to every other page on this website. Please make sure to verify the information with EPFL's official sources.

Ontological neighbourhood

Astronomy

Astrophysics: Stellar astronomy, Physical cosmology

Related lectures (34)