TY  - JOUR
A1  - Niederhofer, Florian
A1  - Cioni, Maria-Rosa L.
A1  - Schmidt, Thomas
A1  - Bekki, Kenji
A1  - de Grijs, Richard
A1  - Ivanov, Valentin D.
A1  - Oliveira, Joana M.
A1  - Ripepi, Vincenzo
A1  - Subramanian, Smitha
A1  - van Loon, Jacco Th
T1  - The VMC survey – XLVI. Stellar proper motions in the centre of the Large Magellanic Cloud
T2  - Monthly notices of the Royal Astronomical Society
N2  - We present proper motion (PM) measurements within the central region of the Large Magellanic Cloud (LMC), using near-infrared data from the VISTA survey of the Magellanic Cloud system (VMC). This work encompasses 18 VMC tiles covering a total sky area of similar to 28 deg(2). We computed absolute stellar PMs from multiepoch observations in the K-s filter over time baselines between similar to 12 and 47 months. Our final catalogue contains similar to 6322 000 likely LMC member stars with derived PMs. We employed a simple flat-rotating disc model to analyse and interpret the PM data. We found a stellar centre of rotation (alpha(0) = 79.95 degrees(+0.22)(-0.23), delta(0) = -69.31 degrees(+0.12)(-0.11)) that is in agreement with that resulting from Hubble Space Telescope data. The inferred viewing angles of the LMC disc (i = 33.5 degrees(+1.2)(-1.3), Theta = 129.8 degrees(+1.9)(-1.9)) are in good agreement with values from the literature but suggest a higher inclination of the central parts of the LMC. Our data confirm a higher rotation amplitude for the young (less than or similar to 0.5 Gyr) stars compared to the intermediate-age/old (greater than or similar to 1 Gyr) population, which can be explained by asymmetric drift. We constructed spatially resolved velocity maps of the intermediate-age/old and young populations. Intermediate-age/old stars follow elongated orbits parallel to the bar's major axis, providing first observational evidence for x(1) orbits within the LMC bar. In the innermost regions, the motions show more chaotic structures. Young stars show motions along a central filamentary bar structure.
KW  - surveys
KW  - proper motion
KW  - stars: kinematics and dynamics
KW  - galaxies: individual: LMC
KW  - Magellanic Clouds
Y1  - 2022
UR  - https://publishup.uni-potsdam.de/frontdoor/index/index/docId/64360
SN  - 0035-8711
SN  - 1365-2966
VL  - 512
IS  - 4
SP  - 5423
EP  - 5439
PB  - Oxford University Press
CY  - Oxford
ER  -