Eclipsing Binaries in Dynamically Interacting Close, Multiple Systems

Close, compact, hierarchical, and multiple stellar systems, i.e., multiples having an outer orbital period from months to a few years, comprise a small but continuously growing group of the triple and multiple star zoo. Many of them consist of at least one eclipsing pair of stars and, therefore, exh...

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Main Author: Tamás Borkovits
Format: Article
Language:English
Published: MDPI AG 2022-01-01
Series:Galaxies
Subjects:
Online Access:https://www.mdpi.com/2075-4434/10/1/9
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author Tamás Borkovits
author_facet Tamás Borkovits
author_sort Tamás Borkovits
collection DOAJ
description Close, compact, hierarchical, and multiple stellar systems, i.e., multiples having an outer orbital period from months to a few years, comprise a small but continuously growing group of the triple and multiple star zoo. Many of them consist of at least one eclipsing pair of stars and, therefore, exhibit readily observable short-term dynamical interactions among the components. Thus, their dynamical and astrophysical properties can be explored with high precision. In this paper we present an overview of the history of the search for additional components around eclipsing binaries from the first serendipitous discoveries to more systematic recent studies. We describe the different observational detection methods and discuss their connections to the different kinds of astrophysical and dynamical information that can be mined from different datasets. Moreover, the connection amongst the observable phenomena and the long-term dynamics of such systems is also discussed.
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spelling doaj.art-7fcdb8376e03499b8f81f135cd31e5732023-11-23T20:00:18ZengMDPI AGGalaxies2075-44342022-01-01101910.3390/galaxies10010009Eclipsing Binaries in Dynamically Interacting Close, Multiple SystemsTamás Borkovits0Baja Astronomical Observatory of University of Szeged, Szegedi út, Kt. 766, H-6500 Baja, HungaryClose, compact, hierarchical, and multiple stellar systems, i.e., multiples having an outer orbital period from months to a few years, comprise a small but continuously growing group of the triple and multiple star zoo. Many of them consist of at least one eclipsing pair of stars and, therefore, exhibit readily observable short-term dynamical interactions among the components. Thus, their dynamical and astrophysical properties can be explored with high precision. In this paper we present an overview of the history of the search for additional components around eclipsing binaries from the first serendipitous discoveries to more systematic recent studies. We describe the different observational detection methods and discuss their connections to the different kinds of astrophysical and dynamical information that can be mined from different datasets. Moreover, the connection amongst the observable phenomena and the long-term dynamics of such systems is also discussed.https://www.mdpi.com/2075-4434/10/1/9binaries: eclipsingbinaries: closestar: multiple
spellingShingle Tamás Borkovits
Eclipsing Binaries in Dynamically Interacting Close, Multiple Systems
Galaxies
binaries: eclipsing
binaries: close
star: multiple
title Eclipsing Binaries in Dynamically Interacting Close, Multiple Systems
title_full Eclipsing Binaries in Dynamically Interacting Close, Multiple Systems
title_fullStr Eclipsing Binaries in Dynamically Interacting Close, Multiple Systems
title_full_unstemmed Eclipsing Binaries in Dynamically Interacting Close, Multiple Systems
title_short Eclipsing Binaries in Dynamically Interacting Close, Multiple Systems
title_sort eclipsing binaries in dynamically interacting close multiple systems
topic binaries: eclipsing
binaries: close
star: multiple
url https://www.mdpi.com/2075-4434/10/1/9
work_keys_str_mv AT tamasborkovits eclipsingbinariesindynamicallyinteractingclosemultiplesystems