Erratum: ``A Radial Velocity Survey of the Cygnus OB2 Association'' (ApJ, 664, 1102 [2007])

Astronomy and Astrophysics – Astrophysics

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The velocity dispersion of Cygnus OB2 was incorrectly quoted in the original manuscript as σV=2.44+/-0.07 km s-1 for Vavg (the weighted average heliocentric velocities), and σV=3.41+/-0.11 km s-1 for Vmid (the averages of the largest and smallest heliocentric velocities). The FWHM values for the Gaussian fits in Figure 23 are also incorrectly quoted as 5.70+/-0.17 km s-1 and 8.01+/-0.26 km s-1 for Vavg and Vmid, respectively. The correct one-dimensional velocity dispersions and corresponding FWHM values, as indicated by the Gaussian fits to the data in Figure 23, are σV=5.74+/-0.15 km s-1 (Vavg), FWHM=13.50+/-0.36 km s-1 (Vavg), σV=8.03+/-0.26 km s-1 (Vmid), and FWHM=18.87+/-0.60 km s-1 (Vmid). These values are larger than typical OB associations and open clusters (1-2.5 km s-1 Bate & Bonnell, ApJ, 664, 1102 [2007]). The larger dispersion estimates may be attributed to the uncertain systemic velocities of binaries (both identified and unidentified), owing to the limited orbital phase information from the current data set.

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