Data Property: spectralPeculiarity
http://www.astro.umd.edu/~eshaya/astro-onto/owl/astronomy.owl#spectralPeculiarity
Annotations
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comment: "Code Spectral peculiarities for stars
: bleeding and/or uncertain spectral value
_ undescribed spectral peculiarities exist
! special peculiarity
comp composite spectrum
e emission lines present
[e] "forbidden" emission lines present
er "reversed" center of emission lines weaker than edges
ep emission lines with peculiarity
eq emission lines with P-Cygni//gr 304.446667, 38.032944 profile
ev spectral emission that exhibits variability
f NIII and HeII emission
(f) weak emission lines of He
((f)) no emission of He
He wk weak He lines
k spectra with interstellar absorption features
m enhanced metal features
n broad ("nebulous") absorption due to spinning
nn very broad absorption features due to spinning very fast
neb a nebula's spectrum mixed in
p peculiar spectrum, strong spectral lines due to metal
pq peculiar spectrum, similar to the spectra of novae
q red and blue shifts line present
s narrowly "sharp" absorption lines
ss very narrow lines
sh shell star
v variable spectral feature (also "var")
w weak lines (also "wl" and "wk")
d Del type A and F giants with weak calcium H and K lines, as in prototype delta Delphini//gr 310.8647916, 15.074694
d Sct type A and F stars with spectra similar to that of short-period variable delta Scuti//gr 280.568417, -9.0525556
Code If spectrum shows enhanced metal features
Ba abnormally strong Barium
Ca abnormally strong Calcium
Cr abnormally strong Chromium
Eu abnormally strong Europium
He abnormally strong Helium
Hg abnormally strong Mercury
Mn abnormally strong Manganese
Si abnormally strong Silicon
Sr abnormally strong Strontium
Code Spectral peculiarities for white dwarfs
P polarized light
H magnetic field from Zeeman splitting
V variable
PEC spetral peculiarities exist" (string)
Domains
Ranges