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xi Tauri: a unique laboratory to study the dynamic interaction in a compact hierarchical quadruple system

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F16%3A10336316" target="_blank" >RIV/00216208:11320/16:10336316 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985815:_____/16:00470536

  • Result on the web

    <a href="http://dx.doi.org/10.1051/0004-0301/2016288" target="_blank" >http://dx.doi.org/10.1051/0004-0301/2016288</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-0301/2016288" target="_blank" >10.1051/0004-0301/2016288</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    xi Tauri: a unique laboratory to study the dynamic interaction in a compact hierarchical quadruple system

  • Original language description

    Context. Compact hierarchical systems are important because the effects caused by the dynamical interaction among its members occur on a human timescale. These interactions play a role in the formation of close binaries through Kozai cycles with tides. One such system is Tauri: it has three hierarchical orbits: 7.14 d (eclipsing components Aa, Ab), 145 d (components Aa+Ab, B), and 51 yr (components Aa+Ab+B, C). Aims. We aim to obtain physical properties of the system and to study the dynamical interaction between its components. Methods. Our analysis is based on a large series of spectroscopic photometric (including space-borne) observations and long-baseline optical and infrared spectro-interferometric observations. We used two approaches to infer the system properties: a set of observation-specific models, where all components have elliptical trajectories, and an N-body model, which computes the trajectory of each component by integrating Newton's equations of motion. Results. The triple subsystem exhibits clear signs of dynamical interaction. The most pronounced are the advance of the apsidal line and eclipse timing variations. We determined the geometry of all three orbits using both observation-specific and N-body models.

  • Czech name

  • Czech description

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

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

    2016

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Astronomy and Astrophysics [online]

  • ISSN

    1432-0746

  • e-ISSN

  • Volume of the periodical

    594

  • Issue of the periodical within the volume

    říjen

  • Country of publishing house

    PL - POLAND

  • Number of pages

    47

  • Pages from-to

  • UT code for WoS article

    000385832200095

  • EID of the result in the Scopus database