Fig. 1.
Single burst model H II LF for
(a) age t = 0; and (b) age t=7 Myr.
The dotted line indicates log lup = 38.48.
The dip near log L ∼ 37.6 is an artifact.
[Note that the slope of log N (log L) vs.
log L is 1-β.]
Fig. 2.
Continuous creation models for
(a) full distribution in N*; and
(b) unsaturated objects with N* ≤ 10
Links (back/forward) to:
| First version: | 20th | March, | 1998
|
| Last update: | 28th | September, | 1998
|
Jochen M. Braun &
Tom Richtler
(E-Mail: jbraun|richtler@astro.uni-bonn.de)
