Binary star database and classification of eclipsing binaries
| Autor: | Malkov, O., Oblak, E., Debray, B. |
|---|---|
| Přispěvatelé: | Institute of Astronomy of the Russian Academy of Sciences (INASAN), Russian Academy of Sciences [Moscow] (RAS), Faculty of Physics, Moscow State University, Univers, Transport, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UMR 6213) (UTINAM), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Franche-Comté (UFC), Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC), J. A. Docobo, R. M. Aller, V. S. Tamazian, Y. Y. Balega, eds. |
| Jazyk: | angličtina |
| Rok vydání: | 2009 |
| Předmět: |
[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] Eclipsing binary stars Astrophysics::Solar and Stellar Astrophysics Astrophysics::Earth and Planetary Astrophysics astronomy databases [PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] catalogs |
| Zdroj: | AIP Conference Proceedings-International Workshop on Double and Multiple Stars: Dynamics, Physics and Instrumentation International Workshop on Double and Multiple Stars: Dynamics, Physics, and Instrumentation International Workshop on Double and Multiple Stars: Dynamics, Physics, and Instrumentation, Dec 2009, Santiago de Compostela, Spain. pp.133-141, ⟨10.1063/1.3597595⟩ |
| DOI: | 10.1063/1.3597595⟩ |
| Popis: | International audience; In this work we present a procedure for the automatic classification of eclipsing binaries. The procedure is based on the data from a new catalogue of 6330 eclipsing variable stars, compiled by the authors and representing the largest list of eclipsing binaries classified from observations. The procedure allows the classification of a given system basing on a set of observational parameters even if the set is incomplete. Results of an application of the procedure to a test sample of a thousand classified systems and to a sample of about five thousand catalogued unclassified systems, as well as to stars from lists of eclipsing variables obtained as by‐products of microlensing surveys (OGLE, MACHO, ASAS‐3), are discussed. The classified eclipsing binaries can be used for determination of astrophysical parameters of their components, and the procedure can be also applied to coming data from future ground‐based and space observatories.The resulting data will be included in the Binary star database, BDB that provides astronomers with the data for binary and multiple stars from all observational categories. We present the current structure of the database and the form and contents of data. We discuss the implementation issues that arise in integrating heterogeneous data sources, the object identifiers problems, interoperability with other databases, implementation of standards for the connection of BDB with International Virtual Observatory, and our future work to extend the capabilities of BDB. |
| Databáze: | OpenAIRE |
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