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Showing 1–4 of 4 results
Advanced filters: Author: Aaron Dotter Clear advanced filters
  • In hierarchical cosmological models, galaxies grow in mass through the continual accretion of smaller ones. The tidal disruption of these systems is expected to result in loosely bound and distant stars surrounding the galaxy. A panoramic survey of the Andromeda galaxy (M31) now reveals stars and coherent structures that are almost certainly remnants of dwarf galaxies destroyed by the tidal field of M31.

    • Alan W. McConnachie
    • Michael J. Irwin
    • Kimberly A. Venn
    Research
    Nature
    Volume: 461, P: 66-69
  • By analysing the chemical abundance differences of pairs of co-moving stars born together, it is found that about 8% show chemical signatures that indicate ingestion of planetary material.

    • Fan Liu
    • Yuan-Sen Ting
    • Fei Dai
    Research
    Nature
    Volume: 627, P: 501-504
  • The observed range of luminosities of the extremely hot ‘blue hook’ stars of the globular cluster ω Centauri is successfully explained by a model in which the progenitors of these stars are second-generation helium-rich stars characterized by a range of rotation rates arising during the cluster’s very early evolution.

    • Marco Tailo
    • Francesca D’Antona
    • Roberto Capuzzo-Dolcetta
    Research
    Nature
    Volume: 523, P: 318-321