Accretion
Accretion is the growth of a massive object by gravitationally attracting more matter in an accretion disc. Accretion discs are common around smaller stars or stellar remnants in a close binary, or black holes in the centers of spiral galaxies. Some dynamics in the disc are necessary to allow orbiting gas to lose angular momentum and fall onto the central massive object. Occasionally, this can result in stellar surface fusion.

Accretion is a collaborative work started by Teurk & Simon Rouby. Depending on the project we also work in unity with artists Boris Maleval, Thomas Hardouin, Kyle Blanton Ross, Benoit Favière, J.B Alazard, Louis Tardivier, Severine Lathuillière, P.E Urcun…

contact us at ferrofluide@gmail.com for any request.