Interstellar objects follow the collapse of molecular clouds

TL;DR

This study demonstrates through simulations that interstellar objects are captured during molecular cloud collapse, influencing the formation and composition of emerging planetary systems.

Contribution

First simulation-based evidence showing ISOs follow molecular cloud collapse and are often gravitationally bound to forming stars.

Findings

At least 40% of sinks have bound ISOs after three free-fall times.

More massive sinks capture larger fractions of ISOs.

Bound ISOs can become unbound if sinks are ejected.

Abstract

Interstellar objects (ISOs), the parent population of 1I/Oumuamua and 2I/Borisov, are abundant in the interstellar medium of the Milky Way. This means that the interstellar medium, including molecular cloud regions, has three components: gas, dust, and ISOs. From the observational constraints for the field density of ISOs drifting in the solar neighbourhood, we infer a typical molecular cloud of 10 pc diameter contains some 10$^{18}$ ISOs. At typical sizes ranging from hundreds of metres to tens of km, ISOs are entirely decoupled from the gas dynamics in these molecular clouds. Here we address the question of whether ISOs can follow the collapse of molecular clouds. We perform low-resolution simulations of the collapse of molecular clouds containing initially static ISO populations toward the point where stars form. In this proof-of-principle study, we find that the interstellar objects definitely follow the collapse of the gas -- and many become bound to the new-forming numerical approximations to future stars (sinks). At minimum, 40\% of all sinks have one or more ISO test particles gravitationally bound to them for the initial ISO distributions tested here. This value corresponds to at least $10^{10}$ actual interstellar objects being bound after three initial free-fall times. Thus, ISOs are a relevant component of star formation. We find that more massive sinks bind disproportionately large fractions of the initial ISO population, implying competitive capture of ISOs. Sinks can also be solitary, as their ISOs can become unbound again -- particularly if sinks are ejected from the system. Emerging planetary systems will thus develop in remarkably varied environments, ranging from solitary to richly populated with bound ISOs.