On the Origin of a Rotating Metal-poor Stellar Population in the Milky Way Nuclear Cluster
Authors: Manuel Arca Sedda, Alessia Gualandris, Tuan Do, Anja Feldmeier-Krause, Nadine Neumayer, and Denis Erkal
2020 The Astrophysical Journal Letters901L29.
Provider: AAS Journals
Caption: Figure D1.
Left (right) panels: combined surface distribution of initial mass and galactocentric distance in the case of an extragalactic origin, assuming an initial eccentricity ﹩{e}_{\mathrm{SC}}=0.5﹩ (0.8).