Multifrequency study of HH 137 and HH 138: Discovering new knots and molecular outflows with Gemini and APEX

TL;DR

This study uses multi-wavelength observations to identify new knots and molecular outflows in HH 137 and HH 138, revealing complex interactions between outflows, shock regions, and molecular clumps, and proposing a scenario linking outflows to dust structures.

Contribution

It provides the first detailed multi-wavelength analysis of HH 137 and HH 138, discovering new shock regions, knots, and outflows, and linking them to molecular clumps and exciting stars.

Findings

Multiple new H$_2$ knots and shock regions identified.

Three molecular outflows associated with optical knots and shock emission.

A molecular clump with an LTE mass of 36 M$_{ ext{⊙}}$ linked to outflows.

Abstract

We present a multi-wavelength study of two HH objects (137 and 138) that may be associated. We use Gemini H$_2$ (2.12 $\mu$m) and K (2.2 $\mu$m) images, as well as APEX molecular line observations and Spitzer image archives. Several H$_2$ knots, linked to the optical chain of knots of HH 137, are identified in the Gemini and Spitzer 4.5 $\mu$m images. New shock excited regions related to the optical knots delineating HH 138 are also reported. In addition, a bright 4.5 $\mu$m 0.09 pc-long arc-shaped structure, roughly located mid-way between HH 137 and HH 138, is found to be associated with two Spitzer Class I/II objects, which are likely to be the exciting stars. These sources are almost coincident with a high-density molecular clump detected in $^{12}$CO(3-2), $^{13}$CO(3-2), C$^{18}$O(3-2), HCO$^{+}$(3-2) and HCN(3-2) molecular lines with an LTE mass of 36 M$_{\odot}$. The $^{12}$CO(3-2) emission distribution over the observed region reveals molecular material underlying three molecular outflows. Two of them (outflows 1 and 2) are linked to all optical knots of HH 137 and HH 138 and to the H$_2$ and 4.5 $\mu$m shock emission knots. In fact, the outflow 2 shows an elongated $^{12}$CO blue lobe that coincides with all the H$_2$ knots of HH 137 which end at a terminal H$_2$ bow shock. We propose a simple scenario that connects the outflows to the dust clumps detected in the region. A third possible outflow is located to the north-east projected towards a secondary weak and cold dust clump.