Stellar wind models of central stars of planetary nebulae

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F20%3A00534348" target="_blank" >RIV/67985815:_____/20:00534348 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1051/0004-6361/201937150" target="_blank" >https://doi.org/10.1051/0004-6361/201937150</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201937150" target="_blank" >10.1051/0004-6361/201937150</a>

Result language
angličtina
Original language name
Stellar wind models of central stars of planetary nebulae
Original language description
We provide global (unified) hot star wind models of central stars of planetary nebulae. The models predict wind structure including the mass-loss rates, terminal velocities, and emergent fluxes from basic stellar parameters. We applied our wind code for parameters corresponding to evolutionary stages between the asymptotic giant branch and white dwarf phases for a star with a final mass of 0.569 M-circle dot. We study the influence of metallicity and wind inhomogeneities (clumping) on the wind properties.
Czech name
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Czech description
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Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)

Project
<a href="/en/project/GA18-05665S" target="_blank" >GA18-05665S: Mass-loss in evolved massive stars</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2020
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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