A search for photometric variability in magnetic chemically peculiar stars using ASAS-3 data
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F15%3A00085398" target="_blank" >RIV/00216224:14310/15:00085398 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1051/0004-6361/201526424" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201526424</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201526424" target="_blank" >10.1051/0004-6361/201526424</a>
Alternative languages
Result language
angličtina
Original language name
A search for photometric variability in magnetic chemically peculiar stars using ASAS-3 data
Original language description
The (magnetic) chemically peculiar (CP) stars of the upper main sequence are well-suited laboratories for investigating the influence of magnetic fields on the stellar surface because they produce abundance inhomogeneities (spots), which results in photometric variability that is explained in terms of the oblique rotator model. CP stars exhibiting this phenomenon are normally classified as alpha2 Canum Venaticorum (ACV) variables. It is important to increase the sample of known rotational periods amongCP stars by discovering new ACV variables. The ASAS-3 data were cross-correlated with the Catalogue of Ap, HgMn, and Am stars in order to analyse the light curves of bona fide CP and related stars. The light curves were downloaded and cleaned of outliersand data points with a flag indicating bad quality. Promising candidates showing a larger scatter than observed for constant stars in the corresponding magnitude range were searched for periodic signals using a standard Fourier technique
Czech name
—
Czech description
—
Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
—
Result continuities
Project
<a href="/en/project/7AMB14AT015" target="_blank" >7AMB14AT015: Shed more light on magnetic stars</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2015
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
ASTRONOMY & ASTROPHYSICS
ISSN
1432-0746
e-ISSN
—
Volume of the periodical
581
Issue of the periodical within the volume
September
Country of publishing house
FR - FRANCE
Number of pages
32
Pages from-to
"nestrankovano"
UT code for WoS article
000361803900138
EID of the result in the Scopus database
—