In this appendix, we give a brief derivation of the frequency integrated
line intensity distribution function, Eq. (73). Similar to the
frequency dependent one, Eq. (61), which is the
starting point of our considerations, we have to account for different regimes,
since the maximum possible (logarithmic) oscillator strength
depends
both on line intensity and frequency. Furthermore, we assume that under
certain circumstances only levels below a cutoff
shall contribute.
In this case then, all lines with lower levels energetically higher than
are neglected. This generalization will turn out to be important if
NLTE-effects are included into our approach (cf. Sect. 4.2.3).
Finally, we allow for an integration between
,
since
for high ionization energies our line list may be incomplete (and
useless, if one accounts for the vanishing flux) beyond a certain maximum
frequency.
At first note, that the maximum possible oscillator strength is given by
![]() |
(E2) |
At low line intensities,
,
we have to
account for the minimum
,
which introduces a threshold frequency
:
By integrating Eq. (61) over frequency and accounting for these
different cases (four in total), we finally obtain the following expressions
for the function F defined in Eq. (73).
![]() |
= | ![]() |
|
![]() |
= | ![]() |
|
![]() |
= | ![]() |
|
![]() |
= | ![]() |
|
![]() |
= | ![]() |
The most important fact concerning the derived function is the following:
Depending on line intensity and the specific value of A, the distribution
can show three different slopes, namely
and
,
where the first one and the last have been found already for
the frequency dependent distribution function (cf. Sect. 4.2.1), whereas the
second one is a new feature arising from the frequency integration.
Let us briefly consider under which condition which slope will show up. At
first, assume that
,
i.e., both the level list and the
line list shall be complete. In this case, Eqs. (E7) and
(E9) have to be applied (
).
For (very) low line intensities, l is approximately
and
.
Thus, the second term in (E7) dominates
and the result is similar to (E6), with maximum frequency
.
In
consequence, F is independent on l and the apparent slope of the
distribution is
(remember, that
). In this situation, for (almost) all possible line
frequencies the contributing oscillator strengths stretch from
to
.
For larger l then,
decreases, whereas
for l
being smaller than
.
We encounter the case that the maximum possible
oscillator strength
can no longer be reached for large frequencies
(cf. Eq. (E4), middle panel), and the apparent slope is controlled by
the sign of A. For negative and not too small A, i.e.,
,
![]() |
(E10) |
For positive A, i.e.,
,
the situation is different. Now the
first bracket of (E7) dominates, giving rise (via the combination
of exponents
)
to an exact
slope of
,
since the dependence on
cancels completely.
This behaviour is finally reached also for negative A and larger l:
For
,
the upper frequential boundary
is
,
which
has the same dependency on l as
.
Additionally, the impact of
small oscillator strengths becomes smaller, simply because the last term in
(E6) decreases with
as function of l.
Nothing changes for negative A and even larger l, when Eq. (E9)
applies. The slope remains at its value .
For positive A,
however, there is a dramatic change for
.
Due to the
interrelation of line intensity and
(cf. the discussion in Sect. 4.2.1),
the dependence on
cancels and only the
slope
survives (the 2nd term in (E9) being now the dominating one). Thus
for
(well) below
the apparent slope at high line intensities
is coupled to the oscillator strength statistics. Finally if
(corresponding to the case A=0 which cannot be treated by the
above formalism), it turns out that the slope at large l
smoothly changes from
to
.
In summary, we have the following behaviour of
if
:
We have considered two case, namely
and 0.93,
respectively, to demonstrate the dependence on
.
In the first case
then,
= 1.46, and the fully drawn line (
)
and the
dotted ones
display the resulting distribution
functions. As predicted by Eq. (E12), the curve for
displays two effective slopes, namely
and
,
where
the dividing line intensity is given by
.
For
,
only one slope (
)
is present due to the third condition
in Eq. (E12). In contrast, the behaviour for
and 3 (
,
Eq. (E11)) depends on
and
,
with a corresponding boundary at
in our example.
For the larger value of
with
,
we see the transition
of slope
to
at
for the
curves with
(dashed-dotted),
and 1.6 (dashed).
Only the case with
reaches its asymptotic value of
,
where also the steeper slope of
for
is clearly visible.
![]() |
Figure E2:
Frequency integrated line intensity distribution function:
variation with
![]() ![]() ![]() ![]() ![]() ![]() ![]() |
In Fig. E2 we demonstrate the influence of either varying the
highest energetic level (
)
or the maximum line frequency (
),
if all other parameters are kept constant. As long as
(dotted curves), the only influence of decreasing
concerns the
region with
,
i.e., Eq. (E6) (partly) replaces
Eq. (E7), where the largest influence is close to
.
Only for very
small values of
the complete first interval is affected. In
consequence, even for
the apparent slope becomes
,
since F depends no longer on l.
In contrast, by diminishing
while keeping
(dashed
curves), the slope of the first interval is barely affected, unless
becomes (very) small compared to
so that the transition value is close
to
(cf. E12, first panel). The major effect of decreasing
,
however, is by shifting the dividing line (which is now a linear
function of
)
to smaller line intensities. Thus, a line-distribution
with
different from
resembles the line-distribution of a
similar ion, however with much smaller ionization energy. This behaviour
turns out to be important if one considers the NLTE line-strength
statistics. Finally, if
approaches zero, the line distribution becomes independent on any excitation
effects. This limiting case, which corresponds to accounting for resonance
lines only, leads to a line-statistics influenced solely by the underlying
gf-distribution.
![]() |
Figure E3:
Frequency integrated line intensity distribution function:
saturation effect. Basic parameters as in Fig. E2.
Fully drawn:
![]() ![]() ![]() ![]() ![]() ![]() |
Figure E3 illustrates the effect of diminishing both
and
.
In principle, the effects are similar to the cases
studied above, namely the transition value is changed via
,
and the
slope of the first region increases to
.
However, there exists
another interesting effect, displayed by the dashed dotted curve: If the
maximum considered frequency
falls below the value of
,
the distribution function becomes "saturated'', i.e., does no longer
change in shape (of course, the absolute value of F and thus the
total line number decreases with
). The reason for this saturation
is given by the fact that Eqs. (E6) and (E8) now control the
behaviour of F, and that for
this function depends on
solely by a constant factor
for all
l.
Note, that in those cases when
is small compared to
(as is
typical under NLTE-conditions, see Sect. 4.2.3), this condition applies for
fairly large
.
In other words: The shape of the
function is the same for all cutoff frequencies smaller than
:
At
maximum two slopes are present, namely either
and
for
or
for
.
This fact
is essential for flux-weighted line-strength distribution function
(Sect. 4.2.8), since the maximum frequency which has to be considered for
this function is fairly small due to the decreasing flux at high energies.
Acknowledgements
We like to thank Ken Gayley, Stan Owocki and Achim Feldmeier for useful comments and suggestions. This project has been supported in part by the Deutsche Forschungsgemeinschaft under DFG grants Pu 117-1/2 and Pa 477-1/2.
Copyright The European Southern Observatory (ESO)