R. Michard, COLOR DISTRIBUTIONS IN E-S0 GALAXIES - III - E-OBJECTS WITH POWER-LAWOR CORE-LIKE CENTRAL PROFILES, Astronomy and astrophysics (Berlin), 335(1), 1998, pp. 49-52
Measurements of the central red color peak occurring in E-type galaxie
s have been obtained from Nieto's CFHT observations in B and R of 39 o
bjects. A careful equalization of the PSF of the two frames involved i
n color maps and profiles was crucial in achieving significant results
, although still affected by limited resolution. The class of the cent
ral light profile, i.e. ''core-like'' or ''power-law'', was also deriv
ed. The well known correlation between the class of central profile an
d the large scale morphology is somewhat improved. The distributions o
f central red peak amplitudes are obtained separately for the two clas
ses of central profiles, and shown to be quite different; most objects
with a core-like center also have a flat central color profile. The m
odel of Silva & Wise (1996), for the production of broad cores by cent
rally located diffuse dust, is not supported. This is in agreement wit
h recent HST results by Carollo et al. (1997) from a special subsample
of objects with kinematically decoupled cores.