Hydrogen.
Unfortunately we have only H
, H
, H
and H
of
the Balmer series. H
is a broad line, about 6000 km
s-1
wide at the continuum level, H
is 2400 km
s-1 wide and
H
1100 km
s-1 wide.
The H
line is too near to the plate limit to be able to say
something meaningful. No line has an indication of a P Cyg structure.
The Paschen series is visible up to n=28, with a clear progression
from n=25 downwards. The emissions are sharp and narrow at our
resolution and show no trace of underlying absorption lines.