We present results from a 36 ks observation of the core of the Pleiades ope
n cluster using ACIS-I on the Chandra X-Ray Observatory. We have detected 5
7 sources, most of which do not have previously known optical counterparts.
Follow-up photometry indicates that many of the detections are likely to b
e active galactic nuclei, in accordance with extragalactic source counts, b
ut some of the sources may be previously undiscovered low-mass members of t
he Pleiades. We discuss our data set and our findings about X-ray emission
from early-type stars, as well as very late-type stars. In particular, the
large X-ray fluxes, lack of variability, and hardness ratios of the four Pl
eiades B6 IV-F4 V stars suggest a tentative conclusion that Pleiades stars
in this spectral type range are intrinsic X-ray sources rather than previou
sly unknown binaries in which the X-ray emission is from a late-type compan
ion. Also, the sensitivity of Chandra allowed us to detect nonflare X-ray e
mission from late M stars.