摘要：Aims. We present a spectroscopic study of the properties of 64 Balmer break galaxies that show signs of star formation. The studied sample of star-forming galaxies spans a redshift range from 0.094 to 1.475 with stellar masses in the range 108–1012M⊙. The sample also includes eight broad emission line galaxies with redshifts between 1.5
关键词：galaxies: evolution;galaxies: star formation;galaxies: high-redshift;galaxies: active;galaxies: stellar content
