1. The mass of the very massive binary WR21a
- Author
-
Laurent Mahy, A. de Koter, Lex Kaper, N. E. Fitzsimons, Frank Tramper, Hugues Sana, A. F. J. Moffat, and Low Energy Astrophysics (API, FNWI)
- Subjects
close [binaries] ,fundamental parameters [stars] ,FOS: Physical sciences ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,spectroscopic [binaries] ,Stellar classification ,01 natural sciences ,Spectral line ,early-type [stars] ,Orbital inclination ,Luminosity ,Primary (astronomy) ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,Binary system ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,Solar and Stellar Astrophysics (astro-ph.SR) ,individual: WR21a [stars] ,Physics ,010308 nuclear & particles physics ,Astronomy ,Astronomy and Astrophysics ,Wolf-Rayet [stars] ,Stars ,Orbit ,Astrophysics - Solar and Stellar Astrophysics ,Space and Planetary Science ,Astrophysics::Earth and Planetary Astrophysics - Abstract
We present multi-epoch spectroscopic observations of the massive binary system WR21a, which include the January 2011 periastron passage. Our spectra reveal multiple SB2 lines and facilitate an accurate determination of the orbit and the spectral types of the components. We obtain minimum masses of $64.4\pm4.8 \ M_{\odot}$ and $36.3\pm1.7 \ M_{\odot}$ for the two components of WR21a. Using disentangled spectra of the individual components, we derive spectral types of O3/WN5ha and O3Vz~((f*)) for the primary and secondary, respectively. Using the spectral type of the secondary as an indication for its mass, we estimate an orbital inclination of $i=58.8\pm2.5^{\mathrm{o}}$ and absolute masses of $103.6\pm10.2 \ M_{\odot}$ and $58.3\pm3.7 \ M_{\odot}$, in agreement with the luminosity of the system. The spectral types of the WR21a components indicate that the stars are very young (1$-$2 Myr), similar to the age of the nearby Westerlund 2 cluster. We use evolutionary tracks to determine the mass-luminosity relation for the total system mass. We find that for a distance of 8 kpc and an age of 1.5 Myr, the derived absolute masses are in good agreement with those from evolutionary predictions., Comment: 7 pages, 4 figures; accepted for publication in MNRAS
- Published
- 2015