Investigating the possible connection between lambda Bootis stars and intermediate Population II type stars
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F14%3A00077782" target="_blank" >RIV/00216224:14310/14:00077782 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1051/0004-6361/201423817" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201423817</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201423817" target="_blank" >10.1051/0004-6361/201423817</a>
Alternative languages
Result language
angličtina
Original language name
Investigating the possible connection between lambda Bootis stars and intermediate Population II type stars
Original language description
The lambda Bootis (LB) stars are located at the upper main sequence of the H-R diagram and exhibit a peculiar abundance pattern. The light elements (C, N, O, and S) present solar abundances whereas all other elements are moderately to strongly underabundant. It has not yet been determined whether that abundance pattern is intrinsic, or is restricted to the stellar surface. If we follow the hypothesis that the LB stars are intrinsically metal-weak, then there should be a connection with the intermediatePopulation II and F-weak objects. Such a possible affinity has not been previously investigated. We present detailed elemental abundances, including those of the light elements carbon and oxygen, for 38 bright intermediate Population II and F-weak objects. In addition, we investigate the kinematic characteristics of the groups. From photometric, spectroscopic, and kinematic data, there is no distinction between the intermediate Population II and F-weak type stars.
Czech name
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Czech description
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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
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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
2014
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
0004-6361
e-ISSN
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Volume of the periodical
567
Issue of the periodical within the volume
7
Country of publishing house
FR - FRANCE
Number of pages
8
Pages from-to
67-74
UT code for WoS article
000341185300121
EID of the result in the Scopus database
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