The properties of energetically unbound stars in stellar clusters

7 Dec 2016Ian ClaydonMark GielesAlice Zocchi

Several Milky Way star clusters show a roughly flat velocity dispersion profile at large radii, which is not expected from models with a tidal cut-off energy. Possible explanations for this excess velocity include: the effects of a dark matter halo, modified gravity theories and energetically unbound stars inside of clusters... (read more)

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