Pulse nav.journalClub Debates activos Tendencias Explorar Investigadores

Join discussions, follow papers, and never miss your next session.

Download on theApp Store

Inicio Explorar nav.journalClub Tendencias

⌘+K

© Synapse Social LLC, 2026

Política de privacidad

August 31, 2009Open Access

Mass accretion rates and histories of dark matter haloes

Puntos clave

Los puntos clave no están disponibles para este artículo en este momento.

Resumen

The mass growth history is a basic property of dark matter haloes. Haloes in numerical simulations are seen to be assembled through a number of processes: mergers with comparable mass haloes (“major mergers”), mergers with smaller

Preguntar a la IA

Me gusta

Guardar

Compartir

Ver artículo completo

Preguntar a la IA

Me gusta

Guardar

Compartir

Ver artículo completo

Cite This Study

McBride et al. (Mon,) studied this question.

synapsesocial.com/papers/69df12d23b0ba53fb37a11e1 https://doi.org/https://doi.org/10.1111/j.1365-2966.2009.15329.x

Also Consider

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

1Populating a cluster of galaxies - I. Results at \fontshape{it}{z}=02001 · 2,698 citations
2The evolution of large-scale structure in a universe dominated by cold dark matter1985 · 3,376 citations
3Constructing Merger Trees that Mimic N-Body Simulations2012 · 85 citations
4Constructing merger trees that mimic N-body simulations2007 · 118 citations
5On halo formation times and assembly bias2008 · 169 citations

Mass accretion rates and histories of dark matter haloes | Synapse