Accurate OH maser positions from the SPLASH pilot region

TL;DR

This study used high-resolution ATCA observations to precisely locate OH masers in the SPLASH pilot region, identifying new sites and classifying their associations with different astrophysical objects.

Contribution

It provides the first high-precision positions for OH masers in the SPLASH pilot region, revealing new sites and improving understanding of their associations with stars, star formation, and remnants.

Findings

Identified 215 OH maser sites, 111 of which are new detections.

57% of sites are associated with evolved stars, 30% with star formation.

Symmetric maser profiles are linked to redder infrared colors, indicating earlier evolutionary stages.

Abstract

We report on high spatial resolution observations, using the Australia Telescope Compact Array (ATCA), of ground-state OH masers. These observations were carried out toward 196 pointing centres previously identified in the Southern Parkes Large-Area Survey in Hydroxyl (SPLASH) pilot region, between Galactic longitudes of $334^{\circ}$ and $344^{\circ}$ and Galactic latitudes of $-2^{\circ}$ and $+2^{\circ}$. Supplementing our data with data from the MAGMO (Mapping the Galactic Magnetic field through OH masers) survey, we find maser emission towards 175 of the 196 target fields. We conclude that about half of the 21 non-detections were due to intrinsic variability. Due to the superior sensitivity of the follow-up ATCA observations, and the ability to resolve nearby sources into separate sites, we have identified 215 OH maser sites towards the 175 fields with detections. Among these 215 OH maser sites, 111 are new detections. After comparing the positions of these 215 maser sites to the literature, we identify 122 (57 per cent) sites associated with evolved stars (one of which is a planetary nebula), 64 (30 per cent) with star formation, two sites with supernova remnants and 27 (13 per cent) of unknown origin. The infrared colors of evolved star sites with symmetric maser profiles tend to be redder than those of evolved star sites with asymmetric maser profiles, which may indicate that symmetric sources are generally at an earlier evolutionary stage.