J/MNRAS/455/1275    Radial velocities of WR21a               (Tramper+, 2016)
The mass of the very massive binary WR21a.
    Tramper F., Sana H., Fitzsimons N.E., de Koter A., Kaper L., Mahy L.,
    Moffat A.
    <Mon. Not. R. Astron. Soc. 455, 1275 (2016)>
    =2016MNRAS.455.1275T 2016MNRAS.455.1275T        (SIMBAD/NED BibCode)
ADC_Keywords: Binaries, spectroscopic ; Stars, Wolf-Rayet ; Radial velocities
Keywords: binaries: close - binaries: spectroscopic - stars: early-type -
          stars: fundamental parameters - stars: individual: WR21a -
          stars: Wolf-Rayet
Abstract:
    We present multi-epoch spectroscopic observations of the massive
    binary system WR21a, which include the 2011 January 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±4.8M_☉ and
    36.3±1.7M_☉ 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±2.5° and
    absolute masses of 103.6±10.2M_☉ and 58.3±3.7M☉, in
    agreement with the luminosity of the system. The spectral types of the
    WR21a components indicate that the stars are very young (1-2Myr),
    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 8kpc and an age
    of 1.5Myr, the derived absolute masses are in good agreement with
    those from evolutionary predictions.
Description:
    All observations of WR21a have been obtained with the X-Shooter
    spectrograph mounted on the European Southern Observatory's VLT. The
    observational campaign has been designed to intensively cover the 2011
    January periastron passage, as well as to provide coverage of the
    orbit on longer time-scales.
Objects:
    -------------------------------------------------------
       RA   (2000)   DE        Designation(s)
    -------------------------------------------------------
    10 25 56.50  -57 48 43.5   WR21a = AX J1025.9-5749
    -------------------------------------------------------
File Summary:
--------------------------------------------------------------------------------
 FileName      Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe            80        .   This file
table1.dat        52       26   Observational log and RV measurements
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Byte-by-byte Description of file: table1.dat
--------------------------------------------------------------------------------
  Bytes Format Units   Label    Explanations
--------------------------------------------------------------------------------
  1-  2  I2    ---     Epoch    Epoch of observation
  4- 12  F9.4  d       HJD      Heliocentric Julian date at mid-exposure
                                 (HJD-2450000)
     14  I1    ---     Nexp     Number of 90s exposures
 16- 19  F4.2  ---     Airmass  Average airmass during observation
 21- 22  I2    ---     SNR      Signal-to-noise ratio per wavelength
                                 bin of 0.2 nm
 24- 28  F5.3  ---     Phase    Orbital phase
 30- 35  F6.1  km/s    RVwr     Radial velocity (RV) of the WR-star component
 37- 40  F4.1  km/s  e_RVwr     1 sigma error on the RV of the WR-star component
 42- 47  F6.1  km/s    RVo      RV of the O-star component
 49- 52  F4.1  km/s  e_RVo      1 sigma error on the RV of the O-star component
--------------------------------------------------------------------------------
Acknowledgements:
     Frank Tramper, F.Tramper(at)uva.nl
(End)     Frank Tramper [UvA, Netherlands], Patricia Vannier [CDS]   09-Feb-2015