Fig. 1.
a) Relative contribution of gaseous emission to broad band colours
UBVRIJHK 1 Myr after the onset of bursts of various
strengths.
b) Decomposition of the total gaseous emission contribution for a strong burst
(Fig. 1a) into contributions from lines and continuum
Fig. 2.
Two colour diagrams for a) (B-V) vs. (V-R) (left or above
panel) and
b) (B-V) vs. (V-K) (right or below panel), respectively
Links (back/forward) to:
First version: | 14th | August, | 1998
|
Last update: | 27th | September, | 1998
|
Jochen M. Braun &
Tom Richtler
(E-Mail: jbraun|richtler@astro.uni-bonn.de)