Hypervelocity runaways from the large magellanic cloud

We explore the possibility that the observed population of Galactic hypervelocity stars (HVSs) originate as runaway stars from the Large Magellanic Cloud (LMC). Pairing a binary evolution code with an N-body simulation of the interaction of the LMC with the Milky Way, we predict the spatial distribu...

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Bibliografski detalji
Glavni autori: Boubert, D, Erkal, D, Evans, N, Izzard, R
Format: Journal article
Jezik:English
Izdano: Oxford University Press 2017