Distance and proper motion measurement of water masers in Shapless 269 IRS 2w
Yoshiharu Asaki, Hiroshi Imai, Andrej Mikhailovich Sobolev, Sergey, Yurievich Parfenov

TL;DR
This study refines the distance and proper motion measurements of water masers in S269 IRS 2w using VLBI data, providing more accurate astrometric parameters and insights into the region's kinematics.
Contribution
The paper presents a new, more reliable parallax measurement of S269 IRS 2w by selecting a better maser feature, improving distance accuracy and kinematic understanding.
Findings
New parallax estimate of 0.247 mas corresponding to 4.05 kpc
Proper motion of (0.39, -1.27) mas/yr determined
Peculiar motion of S269 IRS 2w characterized as (8, -21, 1) km/s
Abstract
We present astrometric analysis of archival data of water masers in the star-forming region Sharpless 269 (S269) IRS 2w, observed with the VLBI Exploration of Radio Astrometry. An annual parallax of one of the bright maser features in this region was previously reported to be 0.189+/-0.008 milliarcsecond (mas) using part of the same archival data as we used. However, we found that this maser feature is not the best to represent the annual parallax to S269 IRS 2w because the morphology is remarkably elongated in the east-west direction. For this study we have selected another maser feature showing simpler morphology. This makes the new annual parallax estimate more credible. Our newly obtained annual parallax is 0.247+/-0.034 mas, corresponding to 4.05+0.65-0.49 kpc. This value is well consistent with the 3.7-3.8 kpc obtained using the kinematic distance estimates and photometric…
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