- ... 18
- Appendices are only available in electronic form at http://www.aanda.org
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- ... acceptable
- In this context,
the H
and He II fluxes are poor selection criteria for
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since the former is proportional to the (unknown) covering factor of the
shell and the latter depends much on questionable synthetic stellar cluster
spectra (Appendix C).
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- ... low
- The tolerance of 9% allowed by SS99 (adopted by V02) is
probably too large (Sect. 3.3). This error bar
is justified in the logic of SS99, who aim to demonstrate an
absence of solution.
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- ... emitted
- SS99 prefer casting
doubt on the ionization balance of S+.
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- ...
- Since [O III]
5007+4959 is exactly matched,
the entry [O III]
4363 in Tables 4 and 5
is the "normalized r([O III])'', i.e., the ratio of the computed r([O III]) to the observed r([O III]).
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- ... for
- LP01 state a priori that [O III]
4363
"almost surely has a contribution from processes other than photoionization''
and conclude that their model "fails to reproduce the observed
[O III]
4363 intensity'', but both statements seem to be refuted
by evidence they present.
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