Article
Model atmosphere analysis of two new early–type O4 dwarfs stars
Authors
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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
D. Fouda, M. Hamdy, M. Nouh, M. Beheary, A. Bakrey and S. M. Saad, “Model atmosphere analysis of two new early–type O4 dwarfs stars,” Applied Mathematics and Nonlinear Sciences, vol. 2, no. 2, pp. 559–564, 2017, doi: 10.21042/AMNS.2017.2.00046.
Fouda D, Hamdy M, Nouh M, Beheary M, Bakrey A, Saad SM. Model atmosphere analysis of two new early–type O4 dwarfs stars. Applied Mathematics and Nonlinear Sciences. 2017;2(2):559–564. doi:10.21042/AMNS.2017.2.00046.
Fouda, D., Hamdy, M., Nouh, M., Beheary, M., Bakrey, A. and Saad, S. M. (2017), ‘Model atmosphere analysis of two new early–type O4 dwarfs stars’, Applied Mathematics and Nonlinear Sciences, 2(2), pp. 559–564. Available at: https://doi.org/10.21042/AMNS.2017.2.00046.
Fouda, D.a., et al. “Model Atmosphere Analysis of Two New Early–type O4 Dwarfs Stars.” Applied Mathematics and Nonlinear Sciences, vol. 2, no. 2, 2017, pp. 559–564. https://doi.org/10.21042/AMNS.2017.2.00046.
Fouda, D.a., M. Hamdy, M. Nouh, M. Beheary, Abdelaziz Bakrey, and S. M. Saad. “Model Atmosphere Analysis of Two New Early–type O4 Dwarfs Stars.” Applied Mathematics and Nonlinear Sciences 2, no. 2 (2017): 559–564. https://doi.org/10.21042/AMNS.2017.2.00046.
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