Year: 2026
Type: article
Abstract: We report the results of a four-epoch very long baseline interferometry experiment targeting seventeen water maser sources in the Magellanic Clouds with the Long Baseline Array. We have measured accurate proper motions for water masers associated with two star formation regions N 180 and N 157A, both in the Large Magellanic Cloud. The water masers have proper motions of left parenthesis 1.79 plus or minus 0.13 comma 0.89 plus or minus 0.03 right parenthesis ( 1.79 ± 0.13 , 0.89 ± 0.03 ) $(1.79\pm{}0.13, 0.89\pm{}0.03)$ milliarcseconds per year and left parenthesis 1.74 plus or minus 0.29 comma 0.55 plus or minus 0.08 right parenthesis ( 1.74 ± 0.29 , 0.55 ± 0.08 ) $(1.74\pm{}0.29, 0.55\pm{}0.08)$ milliarcseconds per year in right ascension and declination, respectively. These results are consistent with the proper motions of nearby stars and the bulk motion of the Large Magellanic Cloud as measured by Gaia, providing independent non-optical evidence of the Large Magellanic Cloud’s motion.
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: hybrid
Estimated APC paid: $3,550
Funder: Australian Research Council
OpenAlex ID: W7170153193
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