VariableTable < Astronome

GCVS variability types in alphabetic order and their corresponding Simbad type(s)

En rose : types pas encore dans Simbad mais qu'on va rajouter; entre {} : type Simbad existant le moins inapproprié en attendant.

En bleu : types GCVS qui n'ont pas d'équivalent dans Simbad mais qu'on ne va pas rajouter

GCVS type	Simbad type	Phenomenological class	Name	Status	Strong emitters
ACEP	Ce*	Pulsating		Evolved; instability strip
ACV	a2*	Rotating	alpha2 CVn variables; magnetic, or Ap stars	Main Sequence	UV
ACVO	a2*	Rotating	Rapidly oscillating alpha2 CVn variables	Main Sequence	UV
ACYG	AC* {sb + Pu}	Pulsating	alpha Cyg variables	Blue supergiant	UV
AM	AM*	Cataclysmic	AM Her, polar, variables	Close binary	X, UV
BCEP	bC*	Pulsating	beta Cep variables	Massive star	UV
BCEPS	bC*	Pulsating	short period beta Cep variables	Massive star	UV
BE	Be*?	?	Be stars	Main Sequence; (can be close binary)	(X, UV, MIR, FIR)
BLBOO	Ce*	Pulsating	anomalous Cepheid variables	Evolved; instability strip
BY	BY*	Rotating (& Eruptive)	BY Dra variables	Main Sequence	X
CEP	Ce*	Pulsating	type I Cepheid variables	Evolved; instability strip
CW	WV*	Pulsating	type II Cepheid variables	Evolved; instability strip
CWA	WV*	Pulsating	W Vir (type II Cepheid) variables	Evolved; instability strip
CWB	WV*	Pulsating	BL Her (type II Cepheid) variables	Evolved; instability strip
DCEP	cC*	Pulsating	delta Cep, classical Cepheid, variables	Evolved; instability strip
DCEPS	cC*	Pulsating	Short period delta Cep variables	Evolved; instability strip
DSCT	dS*	Pulsating	delta Sct variables	Main Sequence	UV
DSCTC	dS*	Pulsating	Low amplitude delta Sct variables	Main Sequence	UV
E	EB*	Binary (eclipsing)	Eclising binaries	Close binary
EA	Al*	Binary (eclipsing)	Algol, beta Per, variables	Detached eclipsing binary
EB	bL*	Binary (eclipsing)	beta Lyr variables	Semi-detached eclipsing binary
EW	WU*	Binary (eclipsing)	W UMa variables	Contact eclipsing binary
ELL	El*	Rotating	ellipsoidal variables	Close binary
EP	EP*	(eclipsing)	Star eclipsed by its planet(s)	Any star
FKCOM	Ro*	Rotating	FK Com variables	?
FU	FU*	Eruptive	FU Ori variables	YSO	X, MIR, FIR
GCAS	Be* + Er*	Eruptive	gamma Cas variables	Binary Be stars with circumstellar outflow	X, UV, MIR, FIR
GDOR	gD*	Pulsating	gamma Dor variables	Main Sequence	UV
I	Ir*	Eruptive	irregular variables
IA	Ir*	Eruptive	irregular variables
IB	Ir*	Eruptive	irregular variables
IN	Or*	Eruptive	Orion variables	YSO	X, MIR, FIR
INA	Or*	Eruptive	Orion variables	YSO	X, MIR, FIR
INB	Or*	Eruptive	Orion variables	YSO	X, MIR, FIR
INT,IT	Or* + TT*	Eruptive	T Tauri variables	YSO	X, MIR, FIR
IN(YY)	Or*	Eruptive	Orion variables	YSO	X, MIR, FIR
INS	Or*	Eruptive	rapid irregular Orion variables	YSO	X, MIR, FIR
IS	RI*	Eruptive	rapid irregular variables
ISA	RI*	Eruptive	rapid irregular variables
ISB	RI*	Eruptive	rapid irregular variables
L	Lr* {LP*}	Pulsating (LPV)	slow irregular variables	Evolved	MIR, (FIR)
LB	Lr* {LP*}	Pulsating (LPV)	slow irregular variables	Evolved; AGB (sometimes red supergiant)	MIR, (FIR)
LC	Lr* {LP*}	Pulsating (LPV)	slow irregular variables	Red supergiant (sometimes AGB)	MIR, (FIR)
M	Mi*	Pulsating (LPV)	Mira variables	Evolved; AGB	MIR, (FIR)
N	CV*	Cataclysmic	Nova candidate	Close binary	X
NA	No*	Cataclysmic	fast Novae	Close binary	X
NB	No*	Cataclysmic	slow Novae	Close binary	X
NC	?	Cataclysmic	Symbiotic	Close binary	X
NL	NL*	Cataclysmic	Novalike	Close binary	X, UV
NR	No*	Cataclysmic	recurrent Novae	Close binary	X
PSR	Psr	Rotating	Pulsar	Neutron star	gam, X, Rad
PVTEL	Pu*	Pulsating	PV tel variables	Blue supergiant
R	CB* {** + V*}	Binary		Close binary
RCB	RC*	Eruptive & Pulsating	R CrB variables	Evolved; H-poor, C-He-rich, luminous	MIR
RR	RR*	Pulsating	RR Lyr variables	Horizontal Branch; instability strip
RRAB	RR*	Pulsating	RR Lyr variables	Horizontal Branch; instability strip
RRC	RR*	Pulsating	RR Lyr variables	Horizontal Branch; instability strip
RPHS	Pu*	Pulsating	Very rapidly pulsating B stars	Subdwarf
LPB	Pu*	Pulsating	"Long"-period pulsating B stars	Subdwarf
RS	RS*	Eruptive & Rotating	RS CVn variables	Close binary	X, UV, MIR
RV	RV*	Pulsating	RV Tau variables	Evolved; post-AGB ?; binary ?	MIR, FIR
RVA	RV*	Pulsating	RV Tau variables	Evolved; post-AGB ?; binary ?	MIR, FIR
RVB	RV*	Pulsating	RV Tau variables	Evolved; post-AGB ?; binary ?	MIR, FIR
SDOR	SD* {sb + Er}	Eruptive	S Dor, Luminous Blue Variables (LBV)	Blue super(hyper)giant	MIR, FIR
SN	SN*	Cataclysmic	Supernovae	Massive star or close binary
SNI	SN*	Cataclysmic	Supernovae of type I	Close binary
SNII	SN*	Cataclysmic	Supernoave of type II	Massive star
SR	sr*	Pulsating (LPV)	Semi-regular variables	Evolved	MIR, (FIR)
SRA	sr*	Pulsating (LPV)	Semi-regular variables	AGB	MIR, (FIR)
SRB	sr*	Pulsating (LPV)	Semi-regular variables	AGB	MIR, (FIR)
SRC	sr*	Pulsating (LPV)	Semi-regular variables	Red supergiant	MIR, (FIR)
SRD	sr*	Pulsating (LPV)	Semi-regular variables	Giant or supergiant with F-G-K spectral type	MIR, (FIR)
SRS	sr*	Pulsating	Semi-regular red giants	RGB (or AGB)	(MIR)
SXARI	ro*	Rotating	SX Ari variables, helium variables	Main sequence
SXPHE	SX*	Pulsating	SX Phe variables	Main sequence, blue straggler
UG	DN*	Cataclysmic	U Gem variables, Dwarf Novae	Close binary	X, UV
UGSS	DN*	Cataclysmic	U Gem variables, Dwarf Novae	Close binary	X, UV
UGSU	DN*	Cataclysmic	U Gem variables, Dwarf Novae	Close binary	X, UV
UGZ	DN*	Cataclysmic	U Gem variables, Dwarf Novae	Close binary	X, UV
UV	Er*	Eruptive	UV Cet variables	YSO	X, MIR, FIR
UVN	Or* + Fl*	Eruptive	Flaring Orion variables	YSO	X, MIR, FIR
WR	WR* + Er*	Eruptive	Eruptive Wolf-Rayet stars	Massive star	X, UV, MIR
X...	XB*	Variable X-ray emission	X-ray binaries	Close binary	X
ZAND	Sy* + CV*	Cataclysmic	Z And variables, symbiotic stars	Close binary	gam, X, UV, MIR, FIR
ZZ	ZZ*	Pulsating	ZZ Cet variables	White dwarf	(X), UV
ZZA	ZZ*	Pulsating	ZZ Cet variables	White dwarf with spectral type DA	(X), UV
ZZB	ZZ*	Pulsating	ZZ Cet variables	White dwarf with spectral type DB	(X), UV
ZZO	ZZ*	Pulsating	ZZ Cet variables	White dwarf with spectral type DO	(X), UV

Type de variables trouvés dans la littérature qui n'existent pas dans le GCVS :

OSARG (OGLE) : LPV + RGB (SRS?)
El CVn : voir 2014MNRAS.437.1681M, type de EB*
AM CVn : type très rare de CV*. Ne pas confondre avec le type AM Her (AM*), même si c'est aussi une CV*.

-- CecileLoup - 2014-05-09

Topic revision: r17 - 2021-09-24 - CecileLoup

Account
- Log In
- Register User

Centre de Données astronomiques de Strasbourg

Edit
Attach