A multi-wavelength analysis of the diffuse HII region G25.8700+0.1350

TL;DR

This study conducts a comprehensive multiwavelength analysis of the HII region G25.8700+0.1350, revealing its structure, distance, associated stellar objects, and potential star formation activity.

Contribution

It provides the first detailed multiwavelength characterization of G25.8700+0.1350, including its structure, stellar content, and star formation indicators, integrating radio, infrared, and molecular data.

Findings

Located at 6.5 kpc distance.

Identified 45 candidate young stellar objects.

Detected associated Wolf-Rayet and red supergiant stars.

Abstract

We present a multiwavelength investigation of the HII region G25.8700+0.1350, located in the inner part of the Galaxy. In radio continuum emission, the region is seen as a bright arc-shaped structure. An analysis of the HI line suggests that G25.8700+0.1350 lies at a distance of 6.5 kpc. The ionized gas is bordered by a photodissociation region which is encircled by a molecular structure where four molecular clumps are detected. At infrared wavelengths, the region is also very conspicuous. Given the high level of visual absorption in the region, the exciting stars should be searched for in the infrared band. In this context, we found in the literature one Wolf-Rayet and one red supergiant which, together with 37 2MASS sources candidates to be O-type stars, could be related to the origin of G25.8700+0.1350. Finally, as expanding HII regions are hypothesized to trigger star formation, we used different infrared point source catalogues to search for young stellar object candidates (cYSOs). A total of 45 cYSOs were identified projected onto the molecular clouds.