Stellar Classification - Spectral Peculiarities

Spectral Peculiarities

Additional nomenclature, in the form of lower-case letters, can follow the spectral type to indicate peculiar features of the spectrum.

Code Spectral peculiarities for stars
: Blending and/or uncertain spectral value
... Undescribed spectral peculiarities exist
! Special peculiarity
comp Composite spectrum
e Emission lines present
"Forbidden" emission lines present
er "Reversed" center of emission lines weaker than edges
ep Emission lines with peculiarity
eq Emission lines with P Cygni profile
ev Spectral emission that exhibits variability
f N III and He II emission (for element name followed by roman numeral see spectral line)
f* NIV λ4058Å is stronger than the NIII λ4634Å, λ4640Å, & λ4642Å lines
f+ SiIV λ4089Å & λ4116Å are emission in addition to the NIII line
(f) N III emission, absence or weak absorption of He II
(f+)
((f)) Displays strong HeII absorption accompanied by weak NIII emissions
((f*))
h WR stars with emission lines due to hydrogen.
ha WR stars with hydrogen emissions seen on both absorption and emission.
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 Unspecified peculiarity, peculiar star.
pq Peculiar spectrum, similar to the spectra of novae
q Red & blue shifts line present
s Narrowly "sharp" absorption lines
ss Very narrow lines
sh Shell star features
v Variable spectral feature (also "var")
w Weak lines (also "wl" & "wk")
d Del Type A and F giants with weak calcium H and K lines, as in prototype Delta Delphini
d Sct Type A and F stars with spectra similar to that of short-period variable Delta Scuti
Code Abnormal CNO features
C C absorption enhanced, N deficient
N N absorption enhanced, C and O deficient
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
Tc Technetium is present
Code Spectral peculiarities for white dwarfs
: Uncertain assigned classification
P Magnetic white dwarf with detectable polarization
E Emission lines present
H Magnetic white dwarf without detectable polarization
V Variable
PEC Spectral peculiarities exist

For example, Epsilon Ursae Majoris is listed as spectral type A0pCr, indicating general classification A0 with strong emission lines of the element chromium. There are several common classes of chemically peculiar stars, where the spectral lines of a number of elements appear abnormally strong.

Read more about this topic:  Stellar Classification

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