Science with an ngVLA: A six-dimensional tomographic view of Galactic star-formation

TL;DR

The paper discusses how the next-generation Very Large Array (ngVLA) will enable precise six-dimensional mapping of star formation in the Milky Way, significantly advancing our understanding of Galactic structure and star-formation processes.

Contribution

It introduces the capabilities of ngVLA for high-precision astrometry across the Galaxy, providing a comprehensive 6D view of star formation.

Findings

ngVLA will improve astrometric sensitivity by over an order of magnitude.

Enables 6D mapping of star-formation regions in the Milky Way.

Transformative potential for understanding Galactic structure.

Abstract

Various sign-posts of recent star-formation activity, such as water and methanol maser emission or magnetically active low-mass young stars, can be detected with Very Long Baseline Interferometry (VLBI) radio arrays. The extremely accurate astrometry already attainable with VLBI instruments implies that the trigonometric parallax and the proper motion of these objects can be measured to better than 1% for sources within a few hundred parsecs of the Sun, and better than 10% for objects at a few kiloparsecs. An ngVLA with baselines extending to several thousand km will have a sensitivity more than one order of magnitude better than current VLBI instruments, and will enable such highly accurate astrometric measurements to be performed throughout the Milky Way. This will provide a full six-dimensional view (three spatial and three velocity coordinates) of star-formation in the Galactic disk, and have a transformative impact on our understanding of both star-formation processes and Galactic structure.