DETERMINATION OF THE TEMPERATURES OF THE CENTRAL STARS OF SELECTED PLANETARY NEBULAE

Abstract

In this work, for planetary nebulae İC 1295, İC 4191, Zanstra temperatures were calculated using the Hβ line of the central stars. Respectively, the temperatures 64252 K and 47663 K were determined. The flux in the Hβ radiative line used in the calculations, has been determined from the spectra retrieved from the archive of the European Southern Observatory. Our results have been compared with results of the other authors.