Spherically Symmetric NLTE Model Atmospheres of Hot Hydrogen-Helium First Stars

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F12%3A00388464" target="_blank" >RIV/67985815:_____/12:00388464 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1088/0067-0049/203/2/20" target="_blank" >http://dx.doi.org/10.1088/0067-0049/203/2/20</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1088/0067-0049/203/2/20" target="_blank" >10.1088/0067-0049/203/2/20</a>

Result language
angličtina
Original language name
Spherically Symmetric NLTE Model Atmospheres of Hot Hydrogen-Helium First Stars
Original language description
We present results of our calculations of NLTE model stellar atmospheres for hot Population III stars composed of hydrogen and helium. We use our own computer code for the calculation of spherically symmetric NLTE model atmospheres in hydrostatic and radiative equilibrium. The model atmospheres are then used for the calculation of emergent fluxes. These fluxes serve to evaluate the flow of high-energy photons for energies higher than ionization energies of hydrogen and helium, the so-called ionizing photon fluxes. We also present the time evolution of the ionizing photon fluxes.
Czech name
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Czech description
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Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Project
<a href="/en/project/GA205%2F08%2F0003" target="_blank" >GA205/08/0003: Mass-loss rate predictions for hot stars</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2012
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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