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[en] A new method is proposed to determine star formation rate, metallicity and initial mass function of stars of a galaxy from its integral energy distribution. The method is applied to the elliptical galaxy NGC 4649 and to the central regions of Sc-galaxies NGC 628, 1637, 4321, 5194
Journal
Pis'ma v Astronomicheskij Zhurnal; ISSN 0320-0108; 
; v. 10(1); p. 19-26
; v. 10(1); p. 19-26