  We performed B and R band surface photometry for E/S0 galaxies in a nearby
rich cluster ABELL 2199 to investigate their B-R color gradients
(d(B-R)/dlogr). Our aims are to study statistical properties of the color
gradients and, by comparing them with those in less dense environments, to
examine environmental dependence of color gradients in elliptical galaxies. We
studied the distribution of the B-R color gradients in the cluster ellipticals
and found that the mean value of the color gradients is -0.09 +- 0.04 mag/dex,
which can be converted to a metallicity gradient (dlogZ/dlogr) of ~ -0.3 +- 0.1
assuming an old stellar population. We further studied the relations between
the B-R color gradients and global properties of the galaxies. Our data suggest
that for the galaxies brighter than L*, more luminous and larger galaxies tend
to have steeper color gradients. The typical value of the color gradients seems
to be consistent with a recent monolithic collapse model and the correlation
could also appear if elliptical galaxies formed through the monolithic
collapse. On the contrary, it is found based on data from the literature that
any such trend is clearly weaker for ellipticals in less dense environments,
while the distribution of the color gradients is quite similar to that found in
the rich cluster. Based on the results from our data and the published data, we
discuss formation process of elliptical galaxy and its environmental
dependence.
