Methanol and water maser observations separate disc and outflow sources in IRAS 19410+2336
M. S. Darwish, K. A. Edris, A. M. S. Richards, S. Etoka, M. S. Saad,, M. M. Beheary, G. A Fuller

TL;DR
This study uses high-resolution maser observations to distinguish between disc and outflow structures in a high-mass star-forming region, revealing complex kinematics and spatial distributions.
Contribution
First astrometric measurements at 6.7 GHz in IRAS 19410+2336, providing detailed maser distributions that differentiate outflow and disc components.
Findings
Methanol masers trace outflows from mm1
Water masers indicate a disc around 13-s
Estimated enclosed mass between 11 and 44 solar masses
Abstract
We investigate the kinematics of high mass protostellar objects within the high mass star forming region IRAS 19410+2336. We performed high angular resolution observations of 6.7-GHz methanol and 22 GHz water masers using the MERLIN (Multi-Element Radio Linked Interferometer Network) and e-MERLIN interferometers. The 6.7-GHz methanol maser emission line was detected within the 16--27 km s velocity range with a peak flux density 50 Jy. The maser spots are spread over 1.3 arcsec on the sky, corresponding to 2800 au at a distance of 2.16 kpc. These are the first astrometric measurements at 6.7 GHz in IRAS 19410+2336. The 22-GHz water maser line was imaged in 2005 and 2019 (the latter with good astrometry). Its velocities range from 13 to 29 km s. The peak flux density was found to be 18.7 Jy and 13.487 Jy in 2005, and 2019, respectively. The…
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