Applied Mathematics and Nonlinear Sciences (Dec 2017)

Model atmosphere analysis of two new early–type O4 dwarfs stars

  • Fouda D.A.,
  • Hamdy M.,
  • Nouh M.,
  • Beheary M.,
  • Bakrey Abdelaziz,
  • Saad S. M.

DOI
https://doi.org/10.21042/AMNS.2017.2.00046
Journal volume & issue
Vol. 2, no. 2
pp. 559 – 564

Abstract

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We present a synthetic spectra study of two new galactic early-type O4 dwarf stars(ALS 19618 and BD+50886) with high signal-to-noise ratio, typically S/N ∼ 300, medium-rosalution R ∼ 2500 optical spectra of O4 dwarfs stars from Galactic O-Stars Spectroscopic Survey (GOSSS), The main stellar parameters (Teff, surface gravity, rotational velocity) have been established using non-LTE, line-blanketed, atmospheric models calculated by TLUSTY204 and SYNSPEC49.

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