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A&A 379, 864-869 (2001)
DOI: 10.1051/0004-6361:20011454
The recent structural evolution of the SMC
F. Maragoudaki1, M. Kontizas1, D. H. Morgan2, E. Kontizas3, A. Dapergolas3 and E. Livanou11 Section of Astrophysics Astronomy & Mechanics, Department of Physics, University of Athens, 15783 Athens, Greece
2 Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, UK
3 Institute of Astronomy and Astrophysics, National Observatory of Athens, PO Box 20048, 11810 Athens, Greece
(Received 28 June 2001 / Accepted 15 October 2001 )
Abstract
We investigate the spatial distribution of stars of different ages towards
the main body of the SMC, in an attempt to further understand the nature
of the complex structure of the SMC.
The old stellar population of the galaxy shows a rather regular and smooth
distribution which is typical for a spheroidal body. On the contrary, the
distribution of the younger stellar component is highly asymmetric and
irregular giving evidence for the severe impact of the SMC during its close
encounter with the LMC some 0.2 to 0.4 Gyr ago.
In a series of isodensity contour maps of stars within selected
ages, the recent structural evolution of the SMC is presented.
Key words: galaxies: Magellanic Clouds -- galaxies: interactions -- galaxies: evolution -- galaxies: structure
Offprint request: F. Maragoudaki, fmarag@cc.uoa.gr
© ESO 2001
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