A spectroscopic study of star clusters and compact emission-line nebulae in NGC 7793

Star clusters and emission-line nebulae are valuable probes of stellar populations and the chemical evolution of nearby galaxies. NGC 7793, the flocculent spiral in the Sculptor Group, contains a rich population of clusters and nebulae, although only a few absorption line objects have been studied spectroscopically so far. Our goal is to confirm the membership of a selected sample of cluster and nebula candidates in NGC 7793 and to derive their main physical and chemical properties. Candidates f