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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

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • 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