Applied Mathematics and Nonlinear Sciences
Journal license

Journal

Applied Mathematics and Nonlinear Sciences


Volume
& Issue

Volume 2, Issue 2


Published
on

December 25, 2017


Pages

559-564


DOI

Article

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

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Authors

D.A. Fouda Affiliation:
National Research Institute of Astronomy and Geophysics (NRIAG), Department of Astronomy, Stellar Lab. Helwan 11421, Cairo. Egypt
, M. Hamdy Affiliation:
National Research Institute of Astronomy and Geophysics (NRIAG), Department of Astronomy, Stellar Lab. Helwan 11421, Cairo. Egypt
, M. Nouh Affiliation:
National Research Institute of Astronomy and Geophysics (NRIAG), Department of Astronomy, Stellar Lab. Helwan 11421, Cairo. Egypt
, M. Beheary Affiliation:
Department of Astronomy and Meteorology, Faculty of Science, El Azhar University, Cairo, Egypt
, Abdelaziz Bakrey Affiliation:
Department of Astronomy and Meteorology, Faculty of Science, El Azhar University, Cairo, Egypt
and S. M. Saad Affiliation:
National Research Institute of Astronomy and Geophysics (NRIAG), Department of Astronomy, Stellar Lab. Helwan 11421, Cairo. Egypt


Abstract

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.


Keywords

Stars: early-type, Stars: dwarfs Stars: Model Atmosphere, Stars: physical parameters, 85A04, 70F15


Citation

Fouda, D., Hamdy, M., Nouh, M., Beheary, M., Bakrey, A., & Saad, S. M. (2017). Model atmosphere analysis of two new early–type O4 dwarfs stars. Applied Mathematics and Nonlinear Sciences, 2(2), 559–564. https://doi.org/10.21042/AMNS.2017.2.00046

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