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Modeling the optical spectra of rho Leo. / Kostenkov, A. ; Batrakov, A. ; Kholtygin, A. ; Valeev, A. .

In: Astronomical Journal of Azerbaijan, Vol. 15, No. 1, 2020, p. 45-47.

Research output: Contribution to journal › Article › peer-review

Harvard

Kostenkov, A, Batrakov, A, Kholtygin, A & Valeev, A 2020, 'Modeling the optical spectra of rho Leo', Astronomical Journal of Azerbaijan, vol. 15, no. 1, pp. 45-47. <http://www.aaj.shao.az/vol15_n1/AAJ_2020_V15_N1.pdf>

APA

Kostenkov, A., Batrakov, A., Kholtygin, A., & Valeev, A. (2020). Modeling the optical spectra of rho Leo. Astronomical Journal of Azerbaijan, 15(1), 45-47. http://www.aaj.shao.az/vol15_n1/AAJ_2020_V15_N1.pdf

Vancouver

Kostenkov A, Batrakov A, Kholtygin A, Valeev A. Modeling the optical spectra of rho Leo. Astronomical Journal of Azerbaijan. 2020;15(1):45-47.

Author

Kostenkov, A. ; Batrakov, A. ; Kholtygin, A. ; Valeev, A. . / Modeling the optical spectra of rho Leo. In: Astronomical Journal of Azerbaijan. 2020 ; Vol. 15, No. 1. pp. 45-47.

BibTeX

@article{502e6e709fa641d0b40685c52a7b5a2d,
title = "Modeling the optical spectra of rho Leo",
abstract = "We present the results of the optical spectroscopic analysis and modeling of B1a star rho Leo. We have analysed spectra of rho Leo obtained with the 6-m BTA telescope (Special Astrophysical Observatory, Nizhnij Arkhyz, Russia) using the SCORPIO focal reducer. We obtain the stellar parameters and chemical abundances of rho Leo comparing models with the observed spectra. Model spectra were calculated using non-local thermodynamic equilibrium (non-LTE) radiative transfer code CMFGEN. We find temperature Teff=23500 K, luminosity L = 2.8E5 Lsun, radius R =31 Rsun, mass M =28 Msun, logg=2.88 and mass-loss rate in the range dM/dt=(9.55-15.00)*E-7 Msun/year. We investigate the impact of an enhanced mass loss rate on the Hbeta, Hgamma, and helium line profiles.",
author = "A. Kostenkov and A. Batrakov and A. Kholtygin and A. Valeev",
year = "2020",
language = "English",
volume = "15",
pages = "45--47",
journal = "Astronomical Journal of Azerbaijan",
issn = "2078-4163",
number = "1",

}

RIS

TY - JOUR

T1 - Modeling the optical spectra of rho Leo

AU - Kostenkov, A.

AU - Batrakov, A.

AU - Kholtygin, A.

AU - Valeev, A.

PY - 2020

Y1 - 2020

N2 - We present the results of the optical spectroscopic analysis and modeling of B1a star rho Leo. We have analysed spectra of rho Leo obtained with the 6-m BTA telescope (Special Astrophysical Observatory, Nizhnij Arkhyz, Russia) using the SCORPIO focal reducer. We obtain the stellar parameters and chemical abundances of rho Leo comparing models with the observed spectra. Model spectra were calculated using non-local thermodynamic equilibrium (non-LTE) radiative transfer code CMFGEN. We find temperature Teff=23500 K, luminosity L = 2.8E5 Lsun, radius R =31 Rsun, mass M =28 Msun, logg=2.88 and mass-loss rate in the range dM/dt=(9.55-15.00)*E-7 Msun/year. We investigate the impact of an enhanced mass loss rate on the Hbeta, Hgamma, and helium line profiles.

AB - We present the results of the optical spectroscopic analysis and modeling of B1a star rho Leo. We have analysed spectra of rho Leo obtained with the 6-m BTA telescope (Special Astrophysical Observatory, Nizhnij Arkhyz, Russia) using the SCORPIO focal reducer. We obtain the stellar parameters and chemical abundances of rho Leo comparing models with the observed spectra. Model spectra were calculated using non-local thermodynamic equilibrium (non-LTE) radiative transfer code CMFGEN. We find temperature Teff=23500 K, luminosity L = 2.8E5 Lsun, radius R =31 Rsun, mass M =28 Msun, logg=2.88 and mass-loss rate in the range dM/dt=(9.55-15.00)*E-7 Msun/year. We investigate the impact of an enhanced mass loss rate on the Hbeta, Hgamma, and helium line profiles.

UR - http://aaj.shao.az/vol15_n1/index.htm

M3 - Article

VL - 15

SP - 45

EP - 47

JO - Astronomical Journal of Azerbaijan

JF - Astronomical Journal of Azerbaijan

SN - 2078-4163

IS - 1

ER -

ID: 71417102