Table 3:

The different variability classes considered by the CVC and our abbreviations.
Stellar variability class Abbreviation
$\beta $-Cephei stars BCEP
Variable Be-stars BE
Classical Cepheids CLCEP
Chemically peculiar stars CP
Double-mode Cepheids DMCEP
$\delta $-Scuti stars DSCUT
Eclipsing binaries (all types) ECL
Ellipsoidal variables ELL
FU-Ori stars FUORI
$\gamma $-Doradus stars GDOR
Herbig Ae/Be stars HAEBE
Low-amplitude periodic variables LAPV
Lambda-Bootis variables LBOO
Luminous Blue variables LBV
Mira variables MIRA
Population II Cepheids PTCEP
Periodically variable supergiants PVSG
RR-Lyrae stars, subtype ab RRAB
RR-Lyrae stars, subtype c RRC
Double-mode RR-Lyrae stars RRD
RV-Tauri stars RVTAU
Pulsating subdwarf B-stars SDBV
Slowly pulsating B-stars SPB
Short-period $\delta $-Scuti variables SPDS
Semi-regular variables SR
SX-Phe stars SXPHE
T-Tauri stars TTAU
Wolf-Rayet stars WR
X-ray binaries XB

Source LaTeX | All tables | In the text

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