More isotopic oblate rotators in elliptical galaxies.

We have extracted from the literature a list of 24 elliptical galaxies showing evidence for having (inner) disks. Reconsidering the (V/σ, ɛ) test, we conclude that kinematical and photometric data (available for 13 galaxies) are consistent with such disk-galaxies being isotropic nearly oblate rotators. We argue that at least about 30 to 50% of genuine E's must have a disk, generally faint, at the low end of the sequence of the disk-to- total luminosity ratio, and are isotropic oblate rotators. Only a favorable orientation reveals the disk in a few of them.