Accretion and Outflows in Young Stars with CUBES

TL;DR

The paper discusses the capabilities of the new CUBES instrument for studying accretion and outflows in low-mass young stellar objects, highlighting its improved sensitivity and potential to extend research to more distant and fainter YSOs.

Contribution

It introduces the high-sensitivity, near-ultraviolet spectrograph CUBES, demonstrating its advantages over current instruments for observing faint and embedded young stellar objects.

Findings

CUBES offers at least four times the spectral resolution of X-Shooter.

Simulations show CUBES can observe YSOs down to V~22 mag in the NUV.

CUBES enables studies of YSOs at kiloparsec distances, expanding the observational horizon.

Abstract

The science case on studies of accretion and outflows in low-mass ($<$1.5 $M_{\odot}$) young stellar objects (YSOs) with the new CUBES instrument is presented. We show the need for a high-sensitivity, near-ultraviolet (NUV) spectrograph like CUBES, with a resolving power at least four times that of X-Shooter and combined with UVES via a fibrelink for simultaneous observations. Simulations with the CUBES exposure time calculator and the end-to-end software show that a significant gain in signal-to -noise can be achieved compared to current instruments, for both the spectral continuum and emission lines, including for relatively embedded YSOs. Our simulations also show that the low-resolution mode of CUBES will be able to observe much fainter YSOs (V $\sim$22 mag) in the NUV than we can today, allowing us extend studies to YSOs with background-limited magnitudes. The performance of CUBES in terms of sensitivity in the NUV will provide important new insights into the evolution of circumstellar disks, by studying the accretion, jets/winds and photo-evaporation processes, down to the low-mass brown dwarf regime. CUBES will also open-up new science as it will be able to observe targets that are several magnitudes fainter than those reachable with current instruments, facilitating studies of YSOs at distances of $\sim$ kpc scale. This means a step-change in the field of low-mass star formation, as it will be possible to expand the science case from relatively local star-forming regions to a large swathe of distances within the Milky Way.