Is sigma Sculptoris Really a Chemically Peculiar Star?

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F15%3A00080770" target="_blank" >RIV/00216224:14310/15:00080770 - 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
Is sigma Sculptoris Really a Chemically Peculiar Star?
Original language description
We have spectroscopically observed the star sigma Scl during two seasons (2011-2012) with the high dispersion spectrograph FEROS (R = 48 000) attached to the 2.2-m MPG/ESO telescope at La Silla. We did not find any spectral changes in a total of 60 obtained spectra. The chemical composition of sigma Scl is very similar to the solar one. We are also unable to find any periodic photometric variations of the star. Consequently, we cannot classify it as a CP star.
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
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>S - Specificky vyzkum na vysokych skolach<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

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
9781583818725
ISSN
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e-ISSN
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Number of pages
6
Pages from-to
197-202
Publisher name
Astronomical Society of the Pacific
Place of publication
San Francisco
Event location
Nizhny Arkhyz, Russia
Event date
Aug 25, 2014
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000366452300024

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