TIC 114936199: A Quadruple Star System with a 12 Day Outer-orbit Eclipse

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F22%3A00563241" target="_blank" >RIV/67985815:_____/22:00563241 - isvavai.cz</a>

Nalezeny alternativní kódy

RIV/47813059:19630/22:A0000199

Výsledek na webu

<a href="https://hdl.handle.net/11104/0337513" target="_blank" >https://hdl.handle.net/11104/0337513</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.3847/1538-4357/ac8934" target="_blank" >10.3847/1538-4357/ac8934</a>

Jazyk výsledku

angličtina

Název v původním jazyce

TIC 114936199: A Quadruple Star System with a 12 Day Outer-orbit Eclipse

Popis výsledku v původním jazyce

We report the discovery with TESS of a remarkable quadruple star system with a 2+1+1 configuration. The two unique characteristics of this system are that (i) the inner eclipsing binary (stars Aa and Ab) eclipses the star in the outermost orbit (star C), and (ii) these outer fourth-body eclipses last for similar to 12 days, the longest of any such system known. The three orbital periods are similar to 3.3 days, similar to 51 days, and similar to 2100 days. The extremely long duration of the outer eclipses is due to the fact that star B slows binary A down on the sky relative to star C. We combine TESS photometric data, ground-based photometric observations, eclipse timing points, radial velocity measurements, the composite spectral energy distribution, and stellar isochrones in a spectrophotodynamical analysis to deduce all of the basic properties of the four stars (mass, radius, T (eff), and age), as well as the orbital parameters for all three orbits. The four masses are M (Aa) = 0.382 M (circle dot), M (Ab) = 0.300 M (circle dot), M (B) = 0.540 M (circle dot), and M (C) = 0.615 M (circle dot), with a typical uncertainty of 0.015 M (circle dot).

Název v anglickém jazyce

TIC 114936199: A Quadruple Star System with a 12 Day Outer-orbit Eclipse

Popis výsledku anglicky

We report the discovery with TESS of a remarkable quadruple star system with a 2+1+1 configuration. The two unique characteristics of this system are that (i) the inner eclipsing binary (stars Aa and Ab) eclipses the star in the outermost orbit (star C), and (ii) these outer fourth-body eclipses last for similar to 12 days, the longest of any such system known. The three orbital periods are similar to 3.3 days, similar to 51 days, and similar to 2100 days. The extremely long duration of the outer eclipses is due to the fact that star B slows binary A down on the sky relative to star C. We combine TESS photometric data, ground-based photometric observations, eclipse timing points, radial velocity measurements, the composite spectral energy distribution, and stellar isochrones in a spectrophotodynamical analysis to deduce all of the basic properties of the four stars (mass, radius, T (eff), and age), as well as the orbital parameters for all three orbits. The four masses are M (Aa) = 0.382 M (circle dot), M (Ab) = 0.300 M (circle dot), M (B) = 0.540 M (circle dot), and M (C) = 0.615 M (circle dot), with a typical uncertainty of 0.015 M (circle dot).

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

—

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2022

Kód důvěrnosti údajů

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

Název periodika

Astrophysical Journal

ISSN

0004-637X

e-ISSN

1538-4357

Svazek periodika

938

Číslo periodika v rámci svazku

2

Stát vydavatele periodika

GB - Spojené království Velké Británie a Severního Irska

Počet stran výsledku

15

Strana od-do

133

Kód UT WoS článku

000870477500001

EID výsledku v databázi Scopus

2-s2.0-85140996600