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We investigate the kinematics of high mass protostellar objects within thehigh mass star forming region IRAS 19410+2336. We performed high angularresolution observations of 6.7-GHz methanol and 22 GHz water masers using theMERLIN (Multi-Element Radio Linked Interferometer Network) and e-MERLINinterferometers. The 6.7-GHz methanol maser emission line was detected withinthe $\sim$ 16--27 km s$^{-1}$ velocity range with a peak flux density $\sim$50Jy. The maser spots are spread over $\sim$1.3 arcsec on the sky, correspondingto $\sim$2800 au at a distance of 2.16 kpc. These are the first astrometricmeasurements at 6.7 GHz in IRAS 19410+2336. The 22-GHz water maser line wasimaged in 2005 and 2019 (the latter with good astrometry). Its velocities rangefrom 13 to $\sim$29 km s$^{-1}$. The peak flux density was found to be 18.7 Jyand 13.487 Jy in 2005, and 2019, respectively. The distribution of the watermaser components is up to 165 mas, $\sim$350 au at 2.16 kpc. We find that theEastern methanol masers most probably trace outflows from the region ofmillimetre source mm1. The water masers to the West lie in a disc (flared orinteracting with outflow/infall) around another more evolved millimetre source(13-s). The maser distribution suggests that the disc lies at an angle of60$^{\circ}$ or more to the plane of the sky and the observed line of sightvelocities then suggest an enclosed mass between 44 M$_{\odot}$ and as littleas 11 M$_{\odot}$ if the disc is edge-on. The Western methanol masers may beinfalling.

Methanol and water maser observations separate disc and outflow sources in IRAS 19410+2336