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

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

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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…

astro-ph2005

Surface density of the young cluster IC 348 in the Perseus molecular cloud

L. Cambresy, V. Petropoulou, M. Kontizas +1

The IC 348 young star cluster contains more than 300 confirmed members. It is embedded in the Perseus molecular cloud, making any clustering analysis subject to an extinction bias.…