Figure 2 from Physics of Galactic Colliders: High-Speed Satellites in ΛCDM Versus Mondian Cosmology

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Physics of Galactic Colliders: High-Speed Satellites in ΛCDM Versus Mondian Cosmology

Authors: Claudio Llinares, HongSheng Zhao, and Alexander Knebe

LLINARES, ZHAO, & KNEBE 2009 The Astrophysical Journal 695 L145.

Provider: AAS Journals

Caption: Figure 2.

Accumulated probability of the relative velocity V _rel between our host halos and their most massive subhalo normalized with the effective dispersion σ _host = 0.01(7.25 M _host,baryon) ^1/3 km s ⁻¹ (see the text for explanation).

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