Capella (alpha Aurigae) Revisited : New Binary Orbit, Physical Properties, and Evolutionary State

Znanstveni rad - Izvorni znanstveni rad

• Autor: G. Torres
• Autor: A. Claret
• Autor: Krešimir Pavlovski
• Autor: A. Dotter
• Autorova ustanova: Sveučilište u Zagrebu; Prirodoslovno-matematički fakultet; (Fizički odsjek)
• Znanstveno / umjetničko područje, polje i grana: PRIRODNE ZNANOSTI; Fizika; Astronomija i astrofizika

Sažetak (engleski)

Knowledge of the chemical composition and absolute masses of Capella are key to understanding the evolutionary state of this benchmark binary system comprising two giant stars. Previous efforts, including our own 2009 study, have largely failed to reach an acceptable agreement between the observations and current stellar evolution models, preventing us from assessing the status of the primary. Here we report a revision of the physical properties of the components incorporating recently published high-precision radial velocity measurements, and a new detailed chemical analysis providing abundances for more than 20 elements in both stars. We obtain highly precise (~0.3%) masses of 2.5687 ± 0.0074 Msun and 2.4828 ± 0.0067 Msun, radii of 11.98 ± 0.57 Rsun and 8.83 ± 0.33 Rsun, effective temperatures of 4970 ± 50 and 5730 ± 60 K, and independently measured luminosities based on the orbital parallax (78.7 ± 4.2 Lsun and 72.7 ± 3.6 Lsun). We find an excellent match to stellar evolution models at the measured composition of [Fe}; ; ; ; /H]=-0.04 ± 0.06. Three different sets of models place the primary star firmly at the end of the core helium-burning phase (clump), while the secondary is known to be evolving rapidly across the Hertzprung gap. The measured lithium abundance, the C/N ratio, and the 12C/13C isotopic carbon abundance ratio, which change rapidly in the giant phase, are broadly in agreement with expectations from models. Predictions from tidal theory for the spin rates, spin–orbit alignment, and other properties do not fare as well, requiring a 40-fold increase in the efficiency of the dissipation mechanisms in order to match the observations.

• Ključne riječi (engleski): binaries: general; binaries: spectroscopic; stars: abundances; stars: evolution; stars: fundamental parameters; stars: individual (Capella)
• Jezik: engleski
• Vrsta publikacije: Znanstveni rad - Izvorni znanstveni rad
• Status objave: Objavljen
• Vrsta recenzije: Recenziran - međunarodna recenzija
• Verzija publikacije: Objavljena verzija rada (izdavačev PDF)
• Naslov časopisa: Astrophysical Journal
• Brojčani podaci: vol. 807, br. 1, A26
• p-ISSN: 0004-637X
• e-ISSN: 1538-4357
• DOI: https://doi.org/10.1088/0004-637X/807/1/26
• URN:NBN: urn:nbn:hr:217:096572
• Datum objave publikacije: 2015
• Projekt: Šifra: IP-2014-09-8656; Naziv (hrvatski): Zvijezde i prašina: struktura, sastav i interakcija; Kratica: STARDUST; Voditelj: Krešimir Pavlovski; Pravna nadležnost: Hrvatska; Financijer: HRZZ; Linija financiranja: IP
• URL dokumenta: https://iopscience.iop.org/article/10.1088/0004-637X/807/1/26
• Vrsta resursa: Tekst
• Prava pristupa: Otvoreni pristup
• Javna napomena: © 2015. The American Astronomical Society. Received 2015 April 29; accepted 2015 May 26; published 2015 June 25.
• Datum i vrijeme pohrane: 2020-01-18 16:50:02