Abstract:
BL Lac objects detected at TeV energies preferentially belong to the subclass called ‘high-frequency-peaked’ BL Lacs (HBLs).
Parsec-scale radio jetsin these TeV-HBLs often show dominant,slow-moving radio knotsthat are at most mildly superluminal. We
report the first systematic campaign to characterize the intranight optical variability (INOV) of TeV-HBLs using a representative
sample of six such sources, all showing a fairly high degree of optical polarization. Our campaign consists of high-sensitivity
monitoring of this sample in 24 sessions of more than 3 h duration each. For these TeV-HBLs, we find a striking lack of INOV
and based on this, we discuss the importance of superluminal motion of the radio knots vis-a-vis the optical polarization, as the
key diagnostic for INOV detection.