Pulsating A-F Stars
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F21%3A00562183" target="_blank" >RIV/67985815:_____/21:00562183 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Pulsating A-F Stars
Original language description
This Chapter provides a brief description of the different classes of pulsating A-F stars emphasising hybrids δ Sct-γ Dor stars. A modelling technique for hybrid δ Sct-γ Dor stars is presented along with the typical features that these stars print on their light curves and frequency spectra. Finally, we present a very different family of pulsating stars overlapping the region where pulsating A-F stars usually lie, the precursors of the so-called extremely low mass white dwarf stars. These stars have very similar atmospheric characteristics and their oscillation periods partially overlap making them diffcult to discern. We discuss tools based on their seismic oscillation properties to distinguish them.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2021
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Pulsations Along Stellar Evolution
ISBN
978-9872494872
ISSN
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e-ISSN
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Number of pages
19
Pages from-to
215-233
Publisher name
Asociación Argentina de Astronomía
Place of publication
La Plata
Event location
La Plata
Event date
Nov 11, 2019
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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