Binary energy source of the HH 250 outflow and its circumstellar environment

TL;DR

This study investigates the binary nature and circumstellar environment of HH 250-IRS, revealing a complex system with a Herbig-Haro flow, multiple disks, and a circumbinary envelope, using multi-wavelength observations.

Contribution

It provides detailed characterization of HH 250-IRS as a binary system with a Herbig-Haro flow, including its disks and circumbinary environment, through comprehensive multi-instrument observations.

Findings

HH 250-IRS is a binary with 120 AU separation.

Both components are Class I sources with different spectral energy distributions.

Gas traces a circumbinary envelope, dust is dominated by one circumstellar envelope.

Abstract

Herbig-Haro flows are signposts of recent major accretion and outflow episodes. We aim to determine the nature and properties of the little-known outflow source HH 250-IRS, which is embedded in the Aquila clouds. We have obtained adaptive optics-assisted L-band images with the NACO instrument on the Very Large Telescope (VLT), together with N- and Q-band imaging with VISIR also on the VLT. Using the SINFONI instrument on the VLT we carried out H- and K-band integral field spectroscopy of HH 250-IRS, complemented with spectra obtained with the SpeX instrument at the InfraRed Telescope Facility (IRTF) in the JHKL bands. Finally, the SubMillimeter Array (SMA) interferometer was used to study the circumstellar environment of HH 250-IRS at 225 and 351 GHz with CO (2-1) and CO (3-2) maps and 0.9 mm and 1.3 mm continuum images. The HH 250-IRS source is resolved into a binary with 0''53 separation, corresponding to 120 AU at the adopted distance of 225 pc. The individual components show heavily veiled spectra with weak CO absorption indicative of late-type stars. Both are Class I sources, but their spectral energy distributions between 1.5 $\mu$m and 19 $\mu$m differ markedly and suggest the existence of a large cavity around one of the components. The millimeter interferometric observations indicate that the gas mainly traces a circumbinary envelope or disk, while the dust emission is dominated by one of the circumstellar envelopes. HH 250-IRS is a new addition to the handful of multiple systems where the individual stellar components, the circumstellar disks and a circumbinary disk can be studied in detail, and a rare case among those systems in which a Herbig-Haro flow is present.