Massive young stellar object W42-MME: The discovery of an infrared jet using VLT/NACO near-infrared images

TL;DR

This paper reports the discovery of an infrared jet from a massive young stellar object in W42, revealing detailed jet-outflow morphology and providing insights into jet formation in massive star formation.

Contribution

The study presents the first detection of a collimated infrared jet from W42-MME using VLT/NACO, along with detailed mapping of its outflow structure and environment.

Findings

Detected a collimated infrared jet within 4500 AU of W42-MME.

Mapped a parsec-scale H2 outflow with bow shocks and specific position angles.

Identified a massive young stellar object with ~19 solar masses.

Abstract

We report on the discovery of an infrared jet from a deeply embedded infrared counterpart of 6.7 GHz methanol maser emission (MME) in W42 (i.e. W42-MME). We also investigate that W42-MME drives a parsec-scale H2 outflow, with detection of bow shock feature at ~0.52 pc to the north. The inner ~0.4 pc part of the H2 outflow has a position angle of ~18 deg and the position angle of ~40 deg is found farther away on either side of outflow from W42-MME. W42-MME is detected at wavelengths longer than 2.2 microns and is a massive young stellar object, with the estimated stellar mass of 19+-4 Msun. We map the inner circumstellar environment of W42-MME using VLT/NACO adaptive optics Ks and L' observations at resolutions ~0.2 arcsec and ~0.1 arcsec, respectively. We discover a collimated jet in the inner 4500 AU using the L' band, which contains prominent Br alpha line emission. The jet is located inside an envelope/cavity (extent ~10640 AU) that is tapered at both ends and is oriented along the north-south direction. Such observed morphology of outflow cavity around massive star is scarcely known and is very crucial for understanding the jet-outflow formation process in massive star formation. Along the flow axis, which is parallel to the previously known magnetic field, two blobs are found in both the NACO images at distances of ~11800 AU, located symmetrically from W42-MME. The observed W42-MME jet-outflow configuration can be used to constrain the jet launching and jet collimation models in massive star formation.