Light Variations of Magnetic Chemically Peculiar Stars

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F15%3A00081638" target="_blank" >RIV/00216224:14310/15:00081638 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Light Variations of Magnetic Chemically Peculiar Stars
Original language description
Light variability of magnetic chemically peculiar stars is caused by the presence of spots with abnormal abundance of some chemical elements on the surface of a rotating star. These abundance spots are being at the same time the photometric features withuneven brightness resulting from an anomalous energy distribution caused by different abundances. We tried to derive the photometric parameters of the spots and determine the intensity distribution inside a spot in the spectral region of 350-550 nm. Wecreated a model for describing the light curves and achieved a good agreement with the observed data. From the simulation of spots we developed a tool deriving the spot parameters directly from the shape of observed mCP light curves.
Czech name
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Czech description
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Project
<a href="/en/project/GA13-10589S" target="_blank" >GA13-10589S: Mass loss in hot massive stars</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>S - Specificky vyzkum na vysokych skolach

Publication year
2015
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
PHYSICS AND EVOLUTION OF MAGNETIC AND RELATED STARS
ISBN
9781583818732
ISSN
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e-ISSN
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Number of pages
9
Pages from-to
230-238
Publisher name
ASTRONOMICAL SOC PACIFIC
Place of publication
SAN FRANCISCO
Event location
Special Astrophys Observ, Nizhny Arkhyz, RUSSIA
Event date
Aug 25, 2014
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000366452300028

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