Astrophysics and Space Science

, Volume 143, Issue 1, pp 99–105

Scanner observations of shell stars ϕ Persei and ψ Persei

  • N. S. Tur
  • P. S. Goraya

DOI: 10.1007/BF00636758

Cite this article as:
Tur, N.S. & Goraya, P.S. Astrophys Space Sci (1988) 143: 99. doi:10.1007/BF00636758


Spectrophotometric energy distribution data of the shell stars ϕ Per and ψ Per are reported in the wavelength range λλ3200–8000 Å. The effective temperature of these stars is derived by comparison of observed energy distribution with theoretical models. Both the stars show higher values of derived effective temperature. The continuum energy distribution in the ultraviolet region has also be discussed.

Copyright information

© Kluwer Academic Publishers 1988

Authors and Affiliations

  • N. S. Tur
    • 1
  • P. S. Goraya
    • 2
  1. 1.Nehru PlanetariumLudhianaIndia
  2. 2.Department of Astronomy and Space SciencesPunjabi UniversityPatialaIndia

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