Science with an ngVLA: New Frontiers in Protostellar Multiplicity with the ngVLA

TL;DR

The ngVLA will revolutionize the study of protostellar multiplicity by enabling detection and resolution of close multiple systems at greater distances, thus advancing understanding of star formation processes.

Contribution

This paper demonstrates the ngVLA's capability to detect and resolve multiple star systems at 1.5 kpc, expanding the scope of multiplicity studies in star-forming regions.

Findings

ngVLA can detect multiple systems at 1.5 kpc

High-resolution imaging reveals close binaries in protostellar environments

Simulations confirm ngVLA's ability to resolve dust emission from binaries

Abstract

The ngVLA will enable significant advances in our understanding of the formation and evolution of multiple star systems in the protostellar phase, building upon the breakthroughs enabled by the VLA. The high-sensitivity and resolution at 3~mm wavelengths and longer will enable closer multiple systems to be discovered in the nearby star forming regions. The ngVLA is incredibly important for multiplicity studies because dust opacity at short wavelengths ($<$3~mm) can hide multiplicity and the long wavelengths are needed to reveal forming multiples in the youngest systems. The samples sizes can be expanded to encompass star forming regions at distances of at least 1.5~kpc, enabling statistical studies that are on par with studies of field star multiplicity. We verify the capability of the ngVLA to detect and resolve multiple star systems at distances out to 1.5~kpc using empirical examples of systems detected by the VLA and scaling them to greater distances. We also use radiative transfer models and simulations to verify that the ngVLA can resolve close binary systems from their dust emission at these distances. The ngVLA will also have excellent imaging capability and the circum-multiple environments can also be examined in great detail.