摘要：After the publication of the original paper of Klement et al.
(2015), a software bug was found in the radiative transfer code
HDUST version 2.02. The error in the code regarded the precise
nature of the photon launching mechanism at the stellar surface
and resulted in slight underestimation of the mean intensities in
the equatorial region, with small but detectable effects in the disk
temperature and emergent spectrum. The new, corrected version
(HDUST 2.10) causes the computed temperature to be slightly
lower and the level populations more neutral. The changes in
the resulting synthetic observables were found to be mostly mi-
nor: a decrease in the level of polarization, line emission, and
the IR flux levels. The effects of the software bug get larger with
increasing stellar rotational velocity.
