Pulsations as a mass-loss trigger in evolved hot stars

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F14%3A00440038" target="_blank" >RIV/67985815:_____/14:00440038 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1017/S174392131301435X" target="_blank" >http://dx.doi.org/10.1017/S174392131301435X</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1017/S174392131301435X" target="_blank" >10.1017/S174392131301435X</a>

Result language
angličtina
Original language name
Pulsations as a mass-loss trigger in evolved hot stars
Original language description
During their post-main sequence evolution, massive stars pass through several short- lived phases, in which they experience enhanced mass loss in the form of clumped winds and mass ejection events of unclear origin. The discovery that stars populating the blue luminous part of the Hertzsprung-Russell diagram can pulsate suggests that stellar pulsations might influence or trigger enhanced mass loss and eruptions. We pre sent recent results for two objects in different phases: a B[e] star at the end of the main sequence and a B-type supergiant.
Czech name
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Czech description
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Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2014
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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