Questions

• Q: Mass segregation? Do you expect such a large number of stars kicked out?
• A: Yes. High density of massive stars in cores, 3-body interaction common there
• Q: NIII and HeII lines? Stellar wind effects move the centroid
• Q: Radial velocities are isolated stars on one side of Arches cluster. Is that expected?
• A: I don't know if we expect that.
• Q: What stellar masses of escaped stars?
• A: Not measured yet.
• A Cornelia: many are radio-continuum detected. Consistent with stellar wind predictions
• Q Farhad: Star formation rate from runaways?
• A: Half of the stars come from clusters. Double the SFR from the clusters. 0.05 Msun/yr
• Q Mark Pound (?): Orbital histories. Are any of the orbits more likely than the others?
• A: Some could have been members.