J/A+A/663/A107         VMC survey XLV.                          (Schmidt+, 2022)

The VMC survey. XLV. Proper motion of the outer LMC and the impact of the SMC. Schmidt T., Cioni M.-R., Niederhofer F., Bekki K., Bell C.P.M., de Grijs R., El Youssoufi D., Ivanov V., Oliveira, J.M., Ripepi V., van Loon J.T. <Astron. Astrophys. 663, A107 (2022)> =2022A&A...663A.107S 2022A&A...663A.107S (SIMBAD/NED BibCode)
ADC_Keywords: Magellanic Clouds ; Associations, stellar ; Proper motions ; Optical Keywords: Galaxy: kinematics and dynamics - Magellanic Clouds - galaxies: interactions - proper motions - surveys Abstract: The Large Magellanic Cloud (LMC) is the most luminous satellite galaxy of the Milky Way and, owing to its companion, the Small Magellanic Cloud (SMC), represents an excellent laboratory to study the interaction of dwarf galaxies. The aim of this study is to investigate the kinematics of the outer regions of the LMC by using stellar proper motions to understand the impact of interactions, e.g. with the SMC about 250Myr ago. We calculate proper motions using multi-epoch Ks-band images from the VISTA survey of the Magellanic Clouds system. Observations span a time baseline of 2-5yr. We combine the VMC data with data from the Gaia early Data Release 3 and introduce a new method to distinguish between Magellanic and Milky Way stars based on a machine learning algorithm. This new technique enables a larger and cleaner sample selection of fainter sources as it reaches below the red clump of the LMC. We investigate the impact of the SMC on the rotational field of the LMC and find hints of stripped SMC debris. The south-eastern region of the LMC shows a slow rotational speed compared to the overall rotation. N-body simulations suggest that this could be caused by a fraction of stripped SMC stars located in that particular region that move opposite to the expected rotation. Description: Tables 5-8 in their entirety for all 257 bins. Columns (from left to right) refer to the bin number as created by the Voronoi routine, right ascension and declination of the bin centre, angular distance of the bin from the LMC centre, number of stars within each bin, their average proper motion in right ascension and declination, and rotational velocity with respect to the LMC centre. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table5.dat 69 258 Gaia EDR3 proper motion of LMC stars table6.dat 69 258 Gaia EDR3 proper motion of old stars table7.dat 69 258 Gaia EDR3 proper motion of young stars table8.dat 69 258 VMC proper motion of LMC stars -------------------------------------------------------------------------------- See also: I/350 : Gaia EDR3 (Gaia Collaboration, 2020) Byte-by-byte Description of file: table5.dat table6.dat table7.dat table8.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Bin Bin number as created by the Voronoi routine 5- 13 F9.6 deg RAdeg Right ascension (ICRS) at Ep=2016.0 of the bin centre (Gaia EDR3) 15- 24 F10.6 deg DEdeg Declination (ICRS) at Ep=2016.0 of the bin centre (Gaia EDR3) 26- 29 F4.2 deg d Angular distance from the LMC centre 31- 35 I5 --- N Number of sources 37- 40 F4.2 mas/yr pmRA Proper motion in Right ascension 42- 45 F4.2 mas/yr e_pmRA Proper motion error in Right ascension 47- 51 F5.2 mas/yr pmDE Proper motion in Declination 53- 56 F4.2 mas/yr e_pmDE Proper motion error in Declination 58- 63 F6.2 km/s VR Rotational velocity with respect to LMC centre 65- 69 F5.2 km/s e_VR Rotational velocity error -------------------------------------------------------------------------------- Acknowledgements: Thomas Schmidt, tschmidt(at)aip.de References: Cioni et al., Paper I 2011A&A...527A.116C 2011A&A...527A.116C, Cat. II/351 Miszalski et al., Paper II 2011A&A...531A.157M 2011A&A...531A.157M, Cat. J/A+A/531/A157 Gullieuszik et al., Paper III 2012A&A...537A.105G 2012A&A...537A.105G, Cat. J/A+A/537/A105 Rubele et al., Paper IV 2012A&A...537A.106R 2012A&A...537A.106R, Ripepi et al., Paper V 2012MNRAS.424.1807R 2012MNRAS.424.1807R, Cat. J/MNRAS/424/1807 Cioni et al., Paper VI 2013A&A...549A..29C 2013A&A...549A..29C, Cat. J/A+A/549/A29 Tatton et al., Paper VII 2013A&A...554A..33T 2013A&A...554A..33T, Cat. J/A+A/554/A33 Ripepi et al., Paper VIII 2014MNRAS.437.2307R 2014MNRAS.437.2307R, Cat. J/MNRAS/437/2307 Cioni et al., Paper IX 2014A&A...562A..32C 2014A&A...562A..32C Moretti et al., Paper X 2014MNRAS.437.2702M 2014MNRAS.437.2702M, Cat. J/MNRAS/437/2702 Li et al., Paper XI 2014ApJ...790...35L 2014ApJ...790...35L Piatti et al., Paper XII 2014A&A...570A..74P 2014A&A...570A..74P Ripepi et al., Paper XIII 2015MNRAS.446.3034R 2015MNRAS.446.3034R, Cat. J/MNRAS/446/3034 Rubele et al., Paper XIV 2015MNRAS.449..639R 2015MNRAS.449..639R, Cat. J/MNRAS/449/639 Piatti et al., Paper XV 2015MNRAS.450..552P 2015MNRAS.450..552P Piatti et al., Paper XVI 2015MNRAS.454..839P 2015MNRAS.454..839P, Cat. J/MNRAS/454/839 Cioni et al., Paper XVII 2016A&A...586A..77C 2016A&A...586A..77C Zhang et al., Paper XVIII 2015ApJ...815...95Z 2015ApJ...815...95Z Ripepi et al., Paper XIX 2016ApJS..224...21R 2016ApJS..224...21R, Cat. J/ApJS/224/21 Moretti et al., Paper XX 2016MNRAS.459.1687M 2016MNRAS.459.1687M, Cat. J/MNRAS/459/1687 Piatti et al., Paper XXI 2016MNRAS.460..383P 2016MNRAS.460..383P Sun et al., Paper XXII 2017ApJ...835..171S 2017ApJ...835..171S Sun et al., Paper XXVII 2017ApJ...849..149S 2017ApJ...849..149S, Cat. J/ApJ/849/149 Marconi et al., Paper XXIII 2017MNRAS.466.3206M 2017MNRAS.466.3206M Subramanian et al., Paper XXIV 2017MNRAS.467.2980S 2017MNRAS.467.2980S Ripepi et al., Paper XXV 2017MNRAS.472..808R 2017MNRAS.472..808R, Cat. J/MNRAS/472/808 Muraveva et al., Paper XXVI 2018MNRAS.473.3131M 2018MNRAS.473.3131M, Cat. J/MNRAS/473/3131 Sun et al., Paper XXVII 2017ApJ...849..149S 2017ApJ...849..149S, Cat. J/ApJ/849/149 Niederhofer et al., Paper XXVIII 2018A&A...612A.115N 2018A&A...612A.115N Sun et al., Paper XXIX 2018ApJ...858...31S 2018ApJ...858...31S, Cat. J/ApJ/858/31 Niederhofer et al., Paper XXX 2018A&A...613L...8N 2018A&A...613L...8N Rubele et al., Paper XXXI 2018MNRAS.478.5017R 2018MNRAS.478.5017R Zivkov et al., Paper XXXII 2018A&A...620A.143Z 2018A&A...620A.143Z Groenewegen et al., Paper XXXIII 2019A&A...622A..63G 2019A&A...622A..63G El Youssoufi et al., Paper XXXIV 2019MNRAS.490.1076E 2019MNRAS.490.1076E Ragosta et al., Paper XXXV 2019MNRAS.490.4975R 2019MNRAS.490.4975R Zivkov et al., Paper XXXVI 2020MNRAS.494..458Z 2020MNRAS.494..458Z, Cat. J/MNRAS/494/458 Groenewegen et al., Paper XXXVII 2020A&A...636A..48G 2020A&A...636A..48G, Cat. J/A+A/636/A48 Schmidt et al., Paper XXXVIII 2020A&A...641A.134S 2020A&A...641A.134S Choudhury et al., Paper XXXIX 2020MNRAS.497.3746C 2020MNRAS.497.3746C Tatton et al., Paper XL 2021MNRAS.504.2983T 2021MNRAS.504.2983T Niederhofer et al., Paper XLI 2021MNRAS.502.2859N 2021MNRAS.502.2859N Cusano et al., Paper XLII 2021MNRAS.504....1C 2021MNRAS.504....1C Mazzi et al., Paper XLIII 2021MNRAS.508..245M 2021MNRAS.508..245M Choudhury et al., Paper XLIV 2021MNRAS.507.4752C 2021MNRAS.507.4752C Miller et al., Paper XLVII 2022MNRAS.512.1196M 2022MNRAS.512.1196M, Cat. J/MNRAS/512/1196
(End) Patricia Vannier [CDS] 31-May-2022
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