Discussion and Analysis

One dimensional spectrum of the inner nebula

 

 

One dimensional spectra of the outer part of the nebula.  Note that the noise is more pronounced because the scale is smaller

 

The two spectra overlaid.  The inner nebula has the larger peaks. 

The Sky Spectrum.  There are a few peaks in regions where there is noise in the other images.

 

Ratio H-alpha:H-beta Ratio OIIIa:OIIIb Ratio H-alpha:OIIIa Ratio H-alpha:HeII Ratio H-alpha:SII Ratio H-alpha:NaI
Inner 5.634 6.132 0.682 14.981 27.523 1.242
Outer 5.599 6.178 0.431 11.925 19.128 15.922
RO/RI 0.994 1.007 0.632 0.796 0.695 12.818
  Inverse Inverse Inverse Inverse Inverse Inverse
Inner 0.178 0.163 1.467 0.067 0.036 0.805
Outer 0.179 0.162 2.319 0.084 0.052 0.063

 

 

Line Actual Wavelength Measured Wavelength
H-alpha 6563 6569.78
H-beta 4861 4863.365
HI/OIII Blend 4340 and 4363 4354.865
OIII 4959 4955.16
OIII 5007 5007.86
SII 6717 and 6731 6733.635
NaI 5890 and 5895 5886.18
HeII 4686 4683.675

 

The HI-gamma/OIII blend is very questionable, particularly since it does not fit the pattern set by the other Hydrogen and Oxygen emission lines.

It is worth noting that if there were any NII emissions at 6548 and 6584 angstroms, they were not resolvable from H-alpha

It may also make sense to discount the NaI ratio, as the peaks were small in the spectra of the inner and outer nebula and could have been greatly affected by sky conditions. 

The measured and actual wavelengths were off in many cases by an inconsistent number - there was no systematic shift in the wavelengths.  However, this did not cause significant difficulty in identifying the lines, since there were rarely other lines in the same region. 

Note that the H-alpha:H-beta ratios are consistent, meaning that reddening is consistent over the entirety of the nebula.  The expected ratio is 2.86 but the actual ratio was about twice that, 5.6, for both the inner and outer, indication that there is in fact reddening occurring.  Because the reddening is consistent and we are concerned with relative prevalence of elemental emissions, the reddening did not affect the results.

 

Conclusions