  We propose a scenario where blazars are classified as flat-spectrum radio
quasars (FSRQs), BL Lacs, low synchrotron, or high synchrotron peaked objects
according to a varying mix of the Doppler boosted radiation from the jet, the
emission from the accretion disk, the broad line region, and the light from the
host galaxy. In this framework the peak energy of the synchrotron power
(nu_peak) in blazars is independent of source type and of radio luminosity. We
test this new approach, which builds upon unified schemes, using extensive
Monte Carlo simulations and show that it can provide simple answers to a number
of long-standing issues including, amongst others, the different cosmological
evolution of BL Lacs selected in the radio and X-ray bands, the larger nu_peak
values observed in BL Lacs, the fact that high synchrotron peaked blazars are
always of the BL Lac type, and the existence of FSRQ/BL Lac transition objects.
Objects so far classified as BL Lacs on the basis of their observed weak, or
undetectable, emission lines are of two physically different classes:
intrinsically weak lined objects, more common in X-ray selected samples, and
heavily diluted broad lined sources, more frequent in radio selected samples,
which explains some of the confusion in the literature. We also show that
strong selection effects are the main cause of the diversity observed in radio
and X-ray samples, and that the correlation between luminosity and nu_peak,
that led to the proposal of the "blazar sequence", is also a selection effect
arising from the comparison of shallow radio and X-ray surveys, and to the fact
that high nu_peak-high radio power objects have never been considered because
their redshift is not measurable.
