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A&A 400, 917-921 (2003)
DOI: 10.1051/0004-6361:20030069
The Small Magellanic Cloud star cluster NGC 458. A new UBVI photometric study
G. Alcaino1, F. Alvarado1, J. Borissova2 and R. Kurtev31 Isaac Newton Institute of Chile, Ministerio de Educacion de Chile, Casilla 8-9, Correo 9, Santiago, Chile
e-mail: inewton@terra.cl
2 Institute of Astronomy, Bulgarian Academy of Sciences and Isaac Newton Institute of Chile Bulgarian Branch, 72 Tsarigradsko chaussèe, 1784 Sofia, Bulgaria
e-mail: jborisso@astro.puc.cl
3 Department of Astronomy, Sofia University and Isaac Newton Institute of Chile Bulgarian Branch, 1164 Sofia, Bulgaria
e-mail: kurtev@phys.uni-sofia.bg
(Received 16 August 2002 / Accepted 7 January 2003 )
Abstract
We present a new photometry of the Small Magellanic Cloud star
cluster NGC 458 in
UBVI filters. We determine the
reddening
. By comparison with the isochrones
by Bertelli et al. (1994) we derive an age of
140 Myr.
Three candidate blue straggler stars are proposed. The evolved "blue loop"
stars of NGC 458 have masses between 4 and 5
and are hotter
than model predictions.
Key words: stars: Hertzsprung-Russell (HR) and C-M diagrams -- galaxies: stellar content -- galaxies: Magellanic clouds -- galaxies: individual: SMC -- galaxies: stars clusters
Offprint request: R. G. Kurtev, kurtev@phys.uni-sofia.bg
SIMBAD Objects
© ESO 2003
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