Fig. 1.
Surface brightness profiles for the BCD galaxies II Zw 33,
Mkn 370 and Mkn 86.
In each pannel it is shown the profile in BVRI filters.
Solid lines are B profiles, long dashed lines correspond to the V
profiles, dotted-dashed lines represent the R and dotted lines show
the I profiles.
Surface magnitude is plotted against, the radius, radius1/4, and
log (R)
Links (back/forward) to:
First version: | 08th | August, | 1998
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Last update: | 29th | September, | 1998
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Jochen M. Braun &
Tom Richtler
(E-Mail: jbraun|richtler@astro.uni-bonn.de)