Automated supervised classification of variable stars in the CoRoT programme - Method and application to the first four exoplanet fields

Free Access

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

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.