paper

Metal Pollution of Low-Mass Population III Stars through Accretion of Interstellar Objects like `Oumuamua

arXiv:1804.08200 · doi:10.1093/pasj/psy075

Abstract

We calculate accretion mass of interstellar objects (ISOs) like `Oumuamua onto low-mass population III stars (Pop.~III survivors), and estimate surface pollution of Pop.~III survivors. An ISO number density estimated from the discovery of `Oumuamua is so high (~au) that Pop.~III survivors have chances at colliding with ISOs times per ~Gyr. `Oumuamua itself would be sublimated near Pop.~III survivors, since it has small size, ~m. However, ISOs with size ~km would reach the Pop.~III survivor surfaces. Supposing an ISO cumulative number density with size larger than is , Pop.~III survivors can accrete ISO mass , or ISO iron mass , if . This iron mass is larger than the accretion mass of interstellar medium (ISM) by several orders of magnitude. Taking into account material mixing in a convection zone of Pop.~III survivors, we obtain their surface pollution is typically [Fe/H] in most cases, however the surface pollution of Pop.~III survivors with can be [Fe/H] because of the very shallow convective layer. If we apply to Pop.III survivors located at the Galactocentric distance of 8 kpc, the dependence of the metal pollustion is as follows. If , Pop.~III survivors have no chance at colliding with ISOs with ~km, and keep metal-free. If , Pop.~III survivors would be most polluted by ISOs up to [Fe/H] . If up to ~km, Pop.~III survivors could hide in metal-poor stars so far discovered. Pop.~III survivors would be more polluted with decreasing the Galactocentric distance. Although the metal pollution depends on and the Galactocentric distance, we first show the importance of ISOs for the metal pollution of Pop.~III survivors.

6 pages, 3 figures, accepted for publication in PASJ