Evidence Suggesting That ‘Oumuamua Is the ∼30 Myr Old Product of a Molecular Cloud
Authors: Cheng-Han Hsieh, Gregory Laughlin, and Héctor G. Arce
2021 The Astrophysical Journal91720.
Provider: AAS Journals
Caption: Figure 6.
The distributions of COL and CAR member stars in position and velocity space relative to the cluster centers. Note that for ‘Oumuamua the ejection velocity is plotted on the y-axis instead of the speed difference from the cluster center.