The peculiar B-type supergiant HD 327083 ?

Coud e spectroscopic data of a poorly-studied peculiar supergiant, HD 327083, are presented. H and H line proles have been tted employing a non-LTE code adequate for spherically expanding atmospheres. Line ts lead to estimates of physical parameters. These parameters suggest that HD 327083 may be close to the Luminous Blue Variable phase but it is also possible that it could be a B(e) Supergiant.