- ... M 33
- Based on
observations obtained at the 4.2 m WHT telescope
operated on the island of La Palma by the Isaac Newton Group in the Spanish
Observatorio del Roque de Los Muchachos of the Instituto de Astrofisica de
Canarias.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... 0.15
- Gurzadyan (1988)
distinguishes between low and high excitation objects.
We prefer to use the term "medium'' instead of low because
when the He II
4686 line is measured the
excitation cannot be really be regarded as low.
We think the specification "low'' is more appropriate for PNe where
the line is not detectable.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.