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S. J. Adelman, “Elemental Abundance Analyses with DAO Spectrograms. VII—The Late Normal B Stars Pi Ceti, 134 Tauri, 21 Aquilae, and Nu Capricorni and the Use of RETICON Spectra,” Monthly Notices of the Royal Astronomical Society, Vol. 252, 1991, pp. 116-131.

has been cited by the following article:

• TITLE: Model Atmosphere Analysis of Some B-Type Stars

  AUTHORS: Somaya M. Saad, Mohamed I. Nouh

  KEYWORDS: B-Type Stars, Model Atmosphere Analysis, Fundamental Parameters

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.1 No.2, July 1, 2011

  ABSTRACT: We present model atmosphere analysis for a sample of B-type stars in optical region to obtain their fundamental parameters e.g. effective temperature, surface gravities, and rotational velocities. Approximate masses for the sample of stars under study are obtained by comparing the resulted effective temperatures and surface gravities with the evolutionary tracks. Comparison between these masses and the empirical effective temperatures-mass relation revealed good agreement.