Article 2022 · 0 atıf

PRECISE MEASUREMENT OF ORBITAL AND PHYSICAL PARAMETERS OF BRIGHT DETACHED SOLAR ANALOG ECLIPSING BINARIES

Cakirli, Omur, Hoyman, Baris, Bulut, Sara, Dervisoglu, Ahmet, Kayhan, Cenk

Özet

We combined photometry from the All Sky Automated Survey (ASAS) and the Transiting Exoplanet Survey Satellite (TESS) with high-resolution spectroscopy from the ESO public archive to obtain, for the first time, absolute physical and orbital parameters for six double-lined detached eclipsing binary systems with solar-type components. The atmospheric parameters of the stars have been determined from the individual spectra obtained with a disentangling method. One of the targets resulted in a triple system, and lines coming from three components in spectra show that each component's contribution to the total light is approximately equal. For the six systems the masses and radii of the components were obtained with a precision better than 3%. A comparison of the observed stellar parameters with the prediction of stellar evolution based on the MESA stellar evolution code shows reasonable agreement.

Anahtar Kelimeler

binaries: eclipsing binaries: spectroscopic stars: evolution stars: fundamental parameters stars: late-type SKY AUTOMATED SURVEY ACCURATE MASSES VARIABLE-STARS CATALOG MULTIPLICITY VELOCITY DISTANCE ELEMENTS SPECTRA QUARTER

WoS Kategorileri

Astronomy & Astrophysics

Künye

Dergi: REVISTA MEXICANA DE ASTRONOMIA Y ASTROFISICA
Yıl: 2022
Cilt: 58
Sayı: 1
Sayfa: 3-21
ISSN: 0185-1101
DOI: 10.22201/ia.01851101p.2022.58.01.01
WoS UID: WOS:000782723100002

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