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arXiv · 1507.06653

HST astrometry in the 30 Doradus region: measuring proper motions of individual stars in the Large Magellanic Cloud

I. Platais·R. P. van der Marel·D. J. Lennon·J. Anderson·A. Bellini·E. Sabbi·H. Sana·L. R. Bedin
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Abstract

We present measurements of positions and relative proper motions in the 30 Doradus region of the Large Magellanic Cloud (LMC). We detail the construction of a single-epoch astrometric reference frame, based on specially-designed observations obtained with the two main imaging instruments ACS/WFC and WFC3/UVIS onboard the Hubble Space Telescope (HST). Internal comparisons indicate a sub milli-arc-second (mas) precision in the positions and the presence of semi-periodic systematics with a mean amplitude of ~0.8 mas. We combined these observations with numerous archival images taken with WFPC2 and spanning 17 years. The precision of the resulting proper motions for well-measured stars around the massive cluster R 136 can be as good as ~20 microarcsec/yr, although the true accuracy of proper motions is generally lower due to the residual systematic errors. The observed proper-motion dispersion for our highest-quality measurements is ~0.1 mas/yr. Our catalog of positions and proper motions contains 86,590 stars down to V~25 and over a total area of ~70 square arcmin. We examined the proper motions of 105 relatively bright stars and identified a total of 6 candidate runaway stars. We are able to tentatively confirm the runaway status of star VFTS 285, consistent with the findings from line-of-sight velocities, and to show that this star has likely been ejected from R 136. This study demonstrates that with HST it is now possible to reliably measure proper motions of individual stars in the nearest dwarf galaxies such as the LMC.

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I. Platais, R. P. van der Marel, D. J. Lennon, J. Anderson, A. Bellini, E. Sabbi, H. Sana, L. R. Bedin. 2015-07-23. HST astrometry in the 30 Doradus region: measuring proper motions of individual stars in the Large Magellanic Cloud. https://doi.org/10.1088/0004-6256%2F150%2F3%2F89

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