The central surface brightness (μV​(0)) of the dwarf spheroidal
satellites of our own Galaxy is found to correlate with their distance from the
Galactic Center (RGC​). This observational evidence suggests that
environmental effects could strongly influence their structure. This suggestion
is further supported by a clear-cut bivariate correlation linking μV​(0) to
a linear combination of MV​, the absolute integrated magnitude, and RGC​,
which seems to be shared also by the M31 spheroidals. Possible implications for
the Fundamental Plane of elliptical galaxies and Dark Matter content of dwarf
spheroidals are also briefly discussed.Comment: 14 pages, plain TEX, 4 figures soon available via
ftp://boas3.bo.astro .it bap/files/ , get bap95-34fig*.ps or
http://www.bo.astro.it/ or upon request at [email protected]
--accepted by MNRAS-Letter