A First Look at the X-ray Population of the Young Massive Cluster VVV CL077

TL;DR

This study presents the first multi-wavelength analysis of the young massive cluster VVV CL077, revealing X-ray emitting stellar members, diffuse X-ray emission, and characteristics consistent with massive O stars, suggesting a distant location in the Norma Arm.

Contribution

First multi-wavelength analysis of VVV CL077, identifying X-ray sources, diffuse emission, and spectral features of massive stars, providing insights into its structure and distance.

Findings

Detected three X-ray stellar members.

Identified diffuse X-ray emission extending from the cluster.

Estimated the cluster's distance and physical properties.

Abstract

Multi-wavelength analysis of the young massive cluster VVV CL077 is presented for the first time. Our Chandra survey of this region enabled the detection of three X-ray emitting stellar members of the cluster, as well as a possible diffuse X-ray component that extends a few arcseconds from the cluster core with an intrinsic flux of (9+/-3)x10^-14 erg cm^-2 s^-1 in the 0.5-10 keV band. Infrared spectra we obtained for two of these X-ray point sources show absorption lines typical of the atmospheres of massive O stars. The X-ray spectrum from the visible extent of VVV CL077 i.e., a 15"-radius around the cluster, can be modeled with an absorbed power law with nH = (6+/-4)x10^22 cm^-2 and gamma = 2+/-1. In addition, the X-ray core of VVV CL077 coincides with diffuse emission seen in the infrared band and with a local maximum in the radio continuum map. A possible association with a neighboring H II region would place VVV CL077 at a distance of around 11 kpc; on the far side of the Norma Arm. At this distance, the cluster is 0.8 pc wide with a mass density of (1-4)x10^3 Msol pc^-3.