Near-Contact Binaries in the Small Magellanic Cloud

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F15%3A00086969" target="_blank" >RIV/00216224:14310/15:00086969 - 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
Near-Contact Binaries in the Small Magellanic Cloud
Original language description
Several thousand eclipsing binaries (EBs) have been found in photometric surveys of the Magellanic Clouds. Periods, amplitudes, and other characteristics of these variable stars have been determined mostly from automatic pipelines, and accurate parameters of the eclipsing pairs and their components are only known for a small fraction of the EBs, mostly for detached ones. We focus on a group of stars in the near contact stage, launching a new project to the improve the accuracy of known parameters and tostudy any (dis)similarities among systems in our Galaxy and in the Magellanic Clouds.
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
LIVING TOGETHER: PLANETS, HOST STARS, AND BINARIES
ISBN
9781583818770
ISSN
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e-ISSN
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Number of pages
3
Pages from-to
223-225
Publisher name
ASTRONOMICAL SOC PACIFIC
Place of publication
SAN FRANCISCO
Event location
Litomysl, CZECH REPUBLIC
Event date
Sep 8, 2014
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000369467900038

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