New Online Database of Symbiotic Variables: [SS2022] 52

Constellation
Sculptor

Equatorial coordinates
α = 00 59 56.976
δ = -33 44 16.831

Galactic coordinates
l = 287.9483°
b = -83.1409°

Suspected	2022^Ref
Confirmed	-
Symbiotic IR type	-
Hot component type	-
Outbursts	-

Identifiers

[SS2022] 52	IRAS F00574-3400	GSC2.4.2 S09V003307	AAVSO -
SIMBAD 2MASS J00595698-3344168	Pan-STARRS 67510149874314670	SAO -	VSX -
GAIA DR3 5003198984975127040	SkyMapper 005956.95-334416.6	WRAY -	GCVS -
2MASS J00595698-3344168	HIP -	Hen -	BD -
WISE J005957.03-334417.3	TYC -	ESO -	HD -

Symbiotic Catalogs

Bidelman (1954)	-	Allen (1984)	-	Belzcyński et al. (2001)	-
Gaposchkin (1957)	-	Kenyon (1986)	-	Akras et al. (2019)	-
Boyarchuk (1969)	-	Vaidis (1988, 1991)	-

Position

Right ascension (°)	14.9874^Ref	Parallax (mas)	0.004±0.118^Ref	Reddening E(B-V) (mag)	0.02±0.0^Ref ^{, Note}
Declination (°)	-33.7380^Ref	Distance (kpc)	5.27^Ref ^{, Note}, 2.22^Ref ^{, Note}
Galactic longitude (°)	287.9483^Ref	Proper motion in α (mas/yr)	-0.07±0.09^Ref
Galactic latitude (°)	-83.1409^Ref	Proper motion in δ (mas/yr)	-0.11±0.07^Ref

Observations

X-Ray	Yes^Ref	IR type	-	Radio	-
X-Ray type	γ or δ^Ref	J (mag)	16.12^Ref	Flickering	-
GALEX FUV (mag)	-	H (mag)	15.48^Ref	Outbursts	-
GALEX NUV (mag)	-	K (mag)	15.39^Ref	Outburst type	-
IUE	No^Ref	WISE W1 (mag)	15.10^Ref	Jets	-
FUSE	No^Ref	WISE W2 (mag)	15.11^Ref	Resolved nebula	-
U (mag)	-	WISE W3 (mag)	12.64^Ref	IPmax (eV)	-
B (mag)	19.54^Ref	WISE W4 (mag)	8.99^Ref	[O III] lines	-
V (mag)	18.27^Ref	IRAS 12μm (Jy)	0.11^Ref	He II lines	-
R (mag)	-	IRAS 25μm (Jy)	0.09^Ref	[Fe VII] lines	-
I (mag)	17.05^Ref	IRAS 60μm (Jy)	0.27^Ref	O VI lines	-
BP (mag)	18.57^Ref	IRAS 100μm (Jy)	0.87^Ref
G (mag)	17.95^Ref	AKARI S09 (Jy)	-
RP (mag)	17.20^Ref	AKARI S18 (Jy)	-

Orbit

Orbital period (days)	-	γ velocity (km/h)	-	Size of giant’s orbit (AU)	-
Eccentricity	-	RV of giant (km/h)	-	Separation (AU)	-
Inclination (°)	-	Inferior conj. of giant (JD)	-	Mass function	-
Eclipses	-			Mass ratio	-
Orbital ephemeris	-

Cool component

Spectral type	-	Mass (M_⊙)	-	Pulsation	-
Eff. temperature (K)	4424±26^Ref	Radius (R_⊙)	-	Type	-
IR type	-	Luminosity (L_⊙)	-	Pulsation period (days)	-
Metallicity [Fe/H]	-1.27^Ref			Pulsation ephemeris	-

Hot component

Type/Spectral type	-	Mass (M_⊙)	-	Spin period (min)	-
Shell-burning/Accreting-only	-	Radius (R_⊙)	-	Accretion disk	-
Eff. temperature (K)	-	Luminosity (L_⊙)	-
Lower limit (K)	-
Upper limit (K)	-

Links

SIMBAD CDS Portal

Notes

The star is suggested as a symbiotic candidate based on the detected X-ray emission and optical/IR counterpart, as reported in Saeedi & Sasaki (2022).

References

Kirby, E. N., Cohen, J. G., Guhathakurta, P. et al., 2013, ApJ, 779, 2, 102, 2013ApJ...779..102K
Saeedi, S., Sasaki, M., 2022, MNRAS, 512, 4, 5481, 2022MNRAS.512.5481S
Skúladóttir, Á., Tolstoy, E., Salvadori, S. et al., 2017, A&A, 606, A71, 2017A&A...606A..71S

[SS2022] 52