Proper motions of spectrally selected structures in the HH 83 outflow

TL;DR

This study measures the proper motions of structures in the HH 83 outflow using Fabry-Perot interferometry over 15 years, revealing a bipolar system, high-velocity differences, and possible outburst history of the source.

Contribution

It provides the first proper motion measurements of spectrally separated structures in HH 83, revealing a bipolar outflow with high velocity differences and evidence of interaction with a dense cloud.

Findings

Discovered a counter bow-shock indicating bipolar symmetry.

Measured proper motions suggesting physical connection between structures.

Indications of outflow-cloud collision and an FU Ori-like outburst 1500 years ago.

Abstract

We continue our program of investigation of the proper motions of spectrally separated structures in the Herbig-Haro outflows with the aid of Fabry-Perot scanning interferometry. This work mainly focuses on the physical nature of various structures in the jets. The aim of the present study is to measure the proper motions of the previously discovered kinematically separated structures in the working surface of the HH 83 collimated outflow. We used observations from two epochs separated by 15 years, which were performed on the 6m telescope with Fabry-Perot scanning interferometer. We obtained images corresponding to different radial velocities for the two separate epochs, and used them to measure proper motions. In the course of our data analysis, we discovered a counter bow-shock of HH 83 flow with positive radial velocity, which makes this flow a relatively symmetric bipolar system. The second epoch observations confirm that the working surface of the flow is split into two structures with an exceptionally large (250 km\ s$^{-1}$) difference in radial velocity. The proper motions of these structures are almost equal, which suggests that they are physically connected. The asymmetry of the bow shock and the turning of proper motion vectors suggests a collision between the outflow and a dense cloud. The profile of the H$\alpha$ line for the directly invisible infrared source HH 83 IRS, obtained by integration of the data within the reflection nebula, suggests it to be of P Cyg type with a broad absorption component characteristic of the FU Ori like objects. If this object underwent an FU Ori type outburst, which created the HH 83 working surfaces, its eruption took place about 1500 years ago according to the kinematical age of the outflow.