Filaments of the Slime Mold Cosmic Web and How They Affect Galaxy Evolution

We present a novel approach for identifying cosmic web filaments within the DisPerSE structure identification framework, using cosmic density field estimates from the Monte Carlo Physarum Machine (MCPM), inspired by the slime mold organism. We apply our method to the IllustrisTNG (TNG100) cosmologic...

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Bibliografske podrobnosti

Principais autores:	Farhanul Hasan, Joseph N. Burchett, Douglas Hellinger, Oskar Elek, Daisuke Nagai, S. M. Faber, Joel R. Primack, David C. Koo, Nir Mandelker, Joanna Woo
Format:	Artigo
Jezik:	Inglês
Izdano:	IOP Publishing 2024-01-01
Serija:	The Astrophysical Journal
Teme:	Galaxy evolution Cosmic web Intergalactic filaments Galaxy quenching Star formation Large-scale structure of the universe
Online dostop:	https://doi.org/10.3847/1538-4357/ad4ee2
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