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20032009
most citedStructure of the SMC - Stellar component distribution from 2MASS data

35 citations · 90 across the 5 of their papers we have counts for

collaborators

8 papers

astro-ph.CO200919 cited

Star complexes and stellar populations in NGC 6822 - Comparison with the Magellanic Clouds

A. Karampelas, A. Dapergolas, E. Kontizas +4

The star complexes (large scale star forming regions) of NGC 6822 were traced and mapped and their size distribution was compared with the size distribution of star complexes in th…

astro-ph200835 cited

Structure of the SMC - Stellar component distribution from 2MASS data

I. Gonidakis, E. Livanou, E. Kontizas +5

The spatial distribution of the SMC stellar component is investigated from 2MASS data. The morphology of the different age populations is presented. The center of the distribution…

astro-ph200723 cited

Towards a library of synthetic galaxy spectra and preliminary results of classification and parametrization of unresolved galaxies for Gaia

P. Tsalmantza, M. Kontizas, C. A. L. Bailer-Jones +8

Aims:The Gaia astrometric survey mission will, as a consequence of its scanning law, obtain low resolution optical (330-1000 nm) spectrophotometry of several million unresolved gal…

astro-ph20078 cited

Star-forming Regions in the Small Magellanic Cloud Multi-wavelength Properties of Stellar Complexes

E. Livanou, I. Gonidakis, E. Kontizas +6

We trace the star formation regions in the SMC and study their properties. The size and spatial distribution of these regions is found to support the hierarchical scenario of star…

astro-ph20065 cited

HST WFPC2 Observations of the Peculiar Main Sequence of the Double Star Cluster NGC 2011 in the Large Magellanic Cloud

D. A. Gouliermis, S. Lianou, M. Kontizas +2

We report the serendipitous discovery of a peculiar main sequence in archived Hubble Space Telescope WFPC2 observations of the young star cluster NGC 2011 in the Large Magellanic C…

astro-ph2005

Star-burst regions in the LMC

E. Livanou, M. Kontizas, I. Gonidakis +5

Aims. Filamentary structures of early type stars are found to be a common feature of the Magellanic Clouds formed at an age of about 0.9-2*10^8 yr. As we go to younger ages these l…