We present a 10-year X-ray light curve and the spectra of a peculiar X-ray
transient in the spiral galaxy M 81. The source was below the detection lim
it of ROSAT PSPC before 1993, but it brightened substantially in 1993, with
luminosities exceeding the Eddington limit of a 1.5-M-. compact accretor.
It then faded and was not firmly detected in the ROSAT HRI and PSPC observa
tions after 1994. The Chandra image obtained in 2000 May, however, shows an
X-ray source at its position within the instrumental uncertainties. The Ch
andra source is coincident with a star-like object in the Digitized-Sky-Sur
vey. A Hubble image suggests that the optical object may be extended. While
these three observations could be of the same object, which may be an X-ra
y binary containing a black-hole candidate, the possibility that the ROSAT
and Chandra sources are two different objects in a dense stellar environmen
t cannot be ruled out. The Hubble data suggests that the optical object may
be a globular cluster yet to be identified.