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Spectrophotometry of three planetary nebulae
Authors:M. A. Kazarian  Elma S. Parsamian  Laura Parrao
Affiliation:(1) Yerevan State University, Armenia;(2) V.A. Ambartsumian Byurakan Astrophysical Observartory, Armenia;(3) Institute of Astronomy of the National Autonomous University of Mexico, USA
Abstract:The results of a spectroscopic investigation of three possible planetary nebulae, K4- 53, K4- 55, and K4- 57, are presented. It is shown that K4- 53 and K4- 55 are planetary nebulae while K4- 57 can be considered with high probability to be one. The temperatures of the nuclei of these nebulae are determined by Ambartsumian’s method. The optical depths for Lc photons in the region of λ ≤ 912 Å are determined. An anomalously high nitrogen abundance is observed in K4- 55.
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