@conference {23844,
	title = {Study of Star Clusters in the Small Magellanic Cloud using the 6.5m Magellan Telescope},
	year = {2013},
	month = {2013/09/1},
	pages = {46 - 46},
	abstract = {We present radial profiles and color magnitude diagrams for 18 star clusters in the central region of the neighboring irregular galaxy Small Magellanic Cloud (SMC), using BVR photometric data obtained with the Inamori Magellan Areal Camera and Spectrograph (IMACS) mounted on the 6.5m Magellan Telescope at the Las Campanas Observatory in Chile. The star clusters studied (OEi79, NGC330, H86- 135, H86-129, H86-127, H86-138, NGC306, H86-146, SOGLE220, B69 OE- SOGLE89, H86-136, H86- 145, BS259, H86-149, H86-142, H86-119, BS257, B73 or SOGLE96) are distributed over a 0.44o field centered at RA: 00h 53m 28.2s, DEC:-72o26?Ao34.5?Ao?Ao (2000) in the central bar and have been previously catalogued by Bonnato \&amp; Bica (2010), Glatt et al. (2010) and Chiosi et al. (2006). The observations obtained with IMACS have very high spatial resolution (of about 0.2 arcsec) and they are thus very well suited for studies of crowded fields. Some of the objects that had been previously classified as clusters in the aforementioned catalogues, have not been confirmed as such, by the new high resolution data. It is also noteworthy that only one of the 18 star clusters has been observed with the Hubble Space Telescope ?Ai and thus with high spatial resolution. For all of the confirmed star clusters in the sample, we have constructed radial density profiles, color magnitude and color-color diagrams. Ages were estimated using the Padova isochrones of Bressan et al. (2012), while the interstellar reddening of each cluster was estimated both from the location of the zero-age main sequence and from the color-color diagrams.},
	url = {https://ui.adsabs.harvard.edu/abs/2013hell.conf...46S},
	author = {Strantzalis, A. and Hatzidimitriou, D. and Antoniou, V. and Zezas, A.}
}
