Near infrared photometric observations (JHKBr) have been made in the field of the galaxy M 83, reaching a magnitude limit K = 20. The quality of data has allowed the systematic search and identification of large numbers of stellar clusters which are intended to determine their fundamental param- eters, as the number of prospective members, reddening, age and luminosity function.
Estudio en el infrarrojo cercano de agrupaciones estelares en M 83
CARRARO, GIOVANNI;
2011
Abstract
Near infrared photometric observations (JHKBr) have been made in the field of the galaxy M 83, reaching a magnitude limit K = 20. The quality of data has allowed the systematic search and identification of large numbers of stellar clusters which are intended to determine their fundamental param- eters, as the number of prospective members, reddening, age and luminosity function.File in questo prodotto:
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