Hostname: page-component-cd9895bd7-lnqnp Total loading time: 0 Render date: 2024-12-25T17:40:19.186Z Has data issue: false hasContentIssue false

Morphology of stellar populations in the Magellanic Clouds using the VMC survey

Published online by Cambridge University Press:  30 October 2019

Dalal El Youssoufi
Affiliation:
Leibniz-Institut für Astrophysik Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
Maria-Rosa L. Cioni
Affiliation:
Leibniz-Institut für Astrophysik Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
Cameron P. M. Bell
Affiliation:
Leibniz-Institut für Astrophysik Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
Stefano Rubele
Affiliation:
Dip. di Fisica e Astronomia, Univ. di Padova, vicolo dell’Osservatorio 2, 35122 Padova, Italy INAF-Osservatorio Astronomico di Padova, vicolo dell’Osservatorio 5, 35122, Padova, Italy
Florian Niederhofer
Affiliation:
Leibniz-Institut für Astrophysik Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
Gal Matijevic
Affiliation:
Leibniz-Institut für Astrophysik Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The Magellanic Clouds are nearby dwarf irregular galaxies that represent a unique laboratory for studying galaxy interactions. Their morphology and dynamics have been heavily influenced by their mutual interactions as well as with their interaction(s) with the Milky Way. We use the VISTA near-infrared YJKs survey of the Magellanic Clouds system (VMC) in combination with stellar partial models of the Large Magellanic Cloud (LMC), the Small Magellanic Cloud (SMC) and the Milky Way to investigate the spatial distribution of stellar populations of different ages across the Magellanic Clouds. In this contribution, we present the results of these studies that allow us to trace substructures possibly related to the interaction history of the Magellanic Clouds.

Type
Contributed Papers
Copyright
© International Astronomical Union 2019 

References

Besla, G., Kallivayalil, N., Hernquist, L., et al. 2007, ApJ, 668, 949 CrossRefGoogle Scholar
Besla, G., Martinez-Delgado, D., van der Marel, R. P., et al. 2016, ApJ, 825, 20 CrossRefGoogle Scholar
Choi, Y., Nidever, D. L., Olsen, K., et al. submitted, arXiv:1805.00481Google Scholar
Cioni, M.-R. L., Habing, H. J., & Israel, F. P. 2000, A&A, 358, L9 Google Scholar
Cioni, M.-R. L., Clementini, G., Girardi, L., et al. 2011, A&A, 527, A116 Google Scholar
Cioni, M.-R. L., Girardi, L., Moretti, M. I., et al. 2014, A&A, 562, A32 Google Scholar
Cioni, M.-R. L., Bekki, K., Girardi, L., et al. 2016, A&A, 586, A77 Google Scholar
de Vaucouleurs, G. & Freeman, K. C 1975, Vistas in Astron., 14, 163 CrossRefGoogle Scholar
Haschke, R., Grebel, E. K., & Duffau, S. 2011, AJ, 141, 158 CrossRefGoogle Scholar
Jacyszyn-Dobrzeniecka, A. M., Skowron, D. M., Mroz, P., et al. 2016, AcA, 66, 149 Google Scholar
Kallivayalil, N., van der Marel, R. P., Alcock, C., et al. 2006, ApJ, 668, 949 Google Scholar
Mackey, D., Koposov, S., Da Costa, G., Belokurov, V., Erkal, D., & Kuzma, P., 2018, ApJ, 858, L21 CrossRefGoogle Scholar
Nikolaev, S. & Weinberg, M. D. 2000, ApJ, 542, 804 CrossRefGoogle Scholar
Nikolaev, S., Drake, A. J., Keller, S. C., et al. 2004, ApJ, 601, 260 CrossRefGoogle Scholar
Olsen, K. A. G. & Salyk, C. 2002, AJ, 124, 2045 CrossRefGoogle Scholar
Rubele, S., Kerber, L., Girardi, L., et al. 2012, A&A, 537, A106 Google Scholar
Scowcroft, V., Freedman, W. L., Madore, B. F., et al. 2016, ApJ, 816, 49 CrossRefGoogle Scholar
Torrealba, G., Koposov, S. E., Belokurov, V., & Irwin, M. 2000, MNRAS, 459, 2370 CrossRefGoogle Scholar
Zaritsky, D., Harris, J., Grebel, E. K., & Thompson, I. B. 2000, ApJ, 534, L53 CrossRefGoogle Scholar