A Binary Nature of the Marginal CP Star Sigma Sculptoris
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F18%3A00100880" target="_blank" >RIV/00216224:14310/18:00100880 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1088/1538-3873/aab142" target="_blank" >http://dx.doi.org/10.1088/1538-3873/aab142</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1088/1538-3873/aab142" target="_blank" >10.1088/1538-3873/aab142</a>
Alternative languages
Result language
angličtina
Original language name
A Binary Nature of the Marginal CP Star Sigma Sculptoris
Original language description
The A2 V star sigma Scl was suspected of being a low-amplitude rotating variable of the Ap-type star by several authors. Aiming to decide whether the star is a variable chemically peculiar (CP) star, we searched for the photometric and spectroscopic variability, and determined chemical abundances of sigma Scl. The possible variability was tested using several types of periodograms applied to the photometry from Long-Term Photometry of Variables project (LTPV) and Hipparcos. Sixty spectrograms of high signal-to-noise (S/N) were obtained and used for chemical analysis of the stellar atmosphere and for looking for spectral variability that is symptomatic for the CP stars. We did not find any signs of the light variability or prominent chemical peculiarity, that is specific for the CP stars. The only exception is the abundance of scandium, which is significantly lower than the solar one and yttrium and barium, which are strongly overabundant. As a by-product of the analysis, and with the addition of 29 further spectra, we found that sigma Scl is a single-lined spectroscopic binary with orbital period of 46.877(8) d. We argue that sigma Scl is not an Ap star, but rather a marginal Am star in SB1 system. The spectral energy distribution of the binary reveals infrared excess due to circumstellar material.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
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)
Others
Publication year
2018
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Publications of the Astronomical Society of the Pacific
ISSN
0004-6280
e-ISSN
1538-3873
Volume of the periodical
130
Issue of the periodical within the volume
987
Country of publishing house
US - UNITED STATES
Number of pages
11
Pages from-to
1-11
UT code for WoS article
000429006800001
EID of the result in the Scopus database
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