Wolf-Rayet stars - what we know and what we don't

Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F24%3A00616839" target="_blank" >RIV/67985815:_____/24:00616839 - isvavai.cz</a>
Výsledek na webu
<a href="https://hdl.handle.net/11104/0363818" target="_blank" >https://hdl.handle.net/11104/0363818</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.59849/2078-4163.2024.2.73" target="_blank" >10.59849/2078-4163.2024.2.73</a>

Jazyk výsledku
angličtina
Název v původním jazyce
Wolf-Rayet stars - what we know and what we don't
Popis výsledku v původním jazyce
Today, we have a sufficiently complete picture of what the Wolf-Rayet (WR) stars are. Predictions of stellar evolution theory are in a good agreement with their parameters, estimated from observational data using stellar atmospheres codes, predictions of population synthesis also agree well with number of known WR stars. This article provides an overview of the main historical milestones in the studies of WR stars, showing how we came to this understanding, and what questions are still unanswered.
Název v anglickém jazyce
Wolf-Rayet stars - what we know and what we don't
Popis výsledku anglicky
Today, we have a sufficiently complete picture of what the Wolf-Rayet (WR) stars are. Predictions of stellar evolution theory are in a good agreement with their parameters, estimated from observational data using stellar atmospheres codes, predictions of population synthesis also agree well with number of known WR stars. This article provides an overview of the main historical milestones in the studies of WR stars, showing how we came to this understanding, and what questions are still unanswered.

Projekt
—
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění
2024
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Podobné výsledky(10)