Possible substellar companions in low-mass eclipsing binaries: GU Bootis and YY Geminorum
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19240%2F18%3AA0000356" target="_blank" >RIV/47813059:19240/18:A0000356 - isvavai.cz</a>
Nalezeny alternativní kódy
RIV/00371912:_____/18:N0000001
Výsledek na webu
<a href="https://www.aanda.org/articles/aa/abs/2018/12/aa33708-18/aa33708-18.html" target="_blank" >https://www.aanda.org/articles/aa/abs/2018/12/aa33708-18/aa33708-18.html</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201833708" target="_blank" >10.1051/0004-6361/201833708</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Possible substellar companions in low-mass eclipsing binaries: GU Bootis and YY Geminorum
Popis výsledku v původním jazyce
We present the next results of our long-term observational project to analyze the variations in the orbital periods of low-mass eclipsing binaries. About 70 new precise mid-eclipse times recorded with a CCD were obtained for two eclipsing binaries with short orbital periods: GU Boo (P = 0.^{d}49) and YY Gem (0.^{d}81). Observed-minus-calculated diagrams of the stars were analyzed using all reliable timings, and new parameters of the light-time effect were obtained. We derived for the first time or improved the short orbital periods of possible third bodies of 11 and 54 years for these low-mass binaries, respectively. We calculated that the minimum masses of the third components are close to 50 M_{Jup}, which corresponds to the mass of brown dwarfs. The multiplicity of these systems also plays an important role in the precise determination of their physical parameters.
Název v anglickém jazyce
Possible substellar companions in low-mass eclipsing binaries: GU Bootis and YY Geminorum
Popis výsledku anglicky
We present the next results of our long-term observational project to analyze the variations in the orbital periods of low-mass eclipsing binaries. About 70 new precise mid-eclipse times recorded with a CCD were obtained for two eclipsing binaries with short orbital periods: GU Boo (P = 0.^{d}49) and YY Gem (0.^{d}81). Observed-minus-calculated diagrams of the stars were analyzed using all reliable timings, and new parameters of the light-time effect were obtained. We derived for the first time or improved the short orbital periods of possible third bodies of 11 and 54 years for these low-mass binaries, respectively. We calculated that the minimum masses of the third components are close to 50 M_{Jup}, which corresponds to the mass of brown dwarfs. The multiplicity of these systems also plays an important role in the precise determination of their physical parameters.
Klasifikace
Druh
J<sub>imp</sub> - Článek v periodiku v databázi Web of Science
CEP obor
—
OECD FORD obor
10308 - Astronomy (including astrophysics,space science)
Návaznosti výsledku
Projekt
—
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2018
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Astronomy & Astrophysics
ISSN
0004-6361
e-ISSN
1432-0746
Svazek periodika
620
Číslo periodika v rámci svazku
December
Stát vydavatele periodika
FR - Francouzská republika
Počet stran výsledku
7
Strana od-do
„A72-1“-„A72-7“
Kód UT WoS článku
000452389400002
EID výsledku v databázi Scopus
2-s2.0-85058064404