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Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?

Fuente: arXiv

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Detalles Bibliográficos
Autores principales:	Porras-Valverde, Antonio J., Forbes, John C., Somerville, Rachel S., Stevens, Adam R. H., Holley-Bockelmann, Kelly, Berlind, Andreas A., Genel, Shy
Formato:	Preprint
Publicado:	2023
Materias:	Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

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