New Online Database of Symbiotic Variables: IGR J17164-3803

Constellation
Scorpius

Equatorial coordinates
α = 17 16 26.943
δ = -38 00 07.538

Galactic coordinates
l = 349.0915°
b = 0.0957°

Suspected	2017^Ref
Confirmed	-
Symbiotic IR type	S?^Ref
Hot component type	accreting-only?^Ref
Outbursts	-

Identifiers

IGR J17164-3803	IRAS 17130-3756	GSC2.4.2 S8BQ016974	AAVSO -
SIMBAD USNO-B1.0 0519-00593639	Pan-STARRS -	SAO -	VSX -
GAIA DR3 5973505420823968640	SkyMapper 171626.94-380007.5	WRAY -	GCVS -
2MASS J17162696-3800075	HIP -	Hen -	BD -
WISE J171627.06-380005.5	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 (°)	259.1123^Ref	Parallax (mas)	0.323±0.053^Ref	Reddening E(B-V) (mag)	31.98±4.49^Ref ^{, Note}
Declination (°)	-38.0021^Ref	Distance (kpc)	3.5^Ref 3.18^Ref ^{, Note}, 2.94^Ref ^{, Note}
Galactic longitude (°)	349.0915^Ref	Proper motion in α (mas/yr)	-2.26±0.06^Ref
Galactic latitude (°)	0.0957^Ref	Proper motion in δ (mas/yr)	-5.72±0.04^Ref

Observations

X-Ray	Yes^Ref	IR type	S?^Ref	Radio	-
X-Ray type	-	J (mag)	8.11^Ref	Flickering	-
GALEX FUV (mag)	-	H (mag)	6.84^Ref	Outbursts	-
GALEX NUV (mag)	-	K (mag)	6.29^Ref	Outburst type	-
IUE	No^Ref	WISE W1 (mag)	5.49^Ref	Jets	-
FUSE	No^Ref	WISE W2 (mag)	5.28^Ref	Resolved nebula	-
U (mag)	-	WISE W3 (mag)	4.64^Ref	IPmax (eV)	-
B (mag)	-	WISE W4 (mag)	2.39^Ref	[O III] lines	-
V (mag)	-	IRAS 12μm (Jy)	13.20^Ref	He II lines	-
R (mag)	-	IRAS 25μm (Jy)	49.30^Ref	[Fe VII] lines	-
I (mag)	-	IRAS 60μm (Jy)	1560.00^Ref	O VI lines	-
BP (mag)	15.23^Ref	IRAS 100μm (Jy)	7110.00^Ref
G (mag)	12.52^Ref	AKARI S09 (Jy)	-
RP (mag)	11.09^Ref	AKARI S18 (Jy)	-

Orbit

Orbital period (days)	-	γ velocity (km/h)	-105.50±0.34^Ref	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	M2^Ref	Mass (M_⊙)	-	Pulsation	-
Eff. temperature (K)	-	Radius (R_⊙)	-	Type	-
IR type	S?^Ref	Luminosity (L_⊙)	-	Pulsation period (days)	-
Metallicity [Fe/H]	-			Pulsation ephemeris	-

Hot component

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

Links

SIMBAD CDS Portal

Notes

Identified as an X-ray source, it was suggested to be a symbiotic star by Rahoui et al. (2017). The optical counterpart was identified as USNOB1.0 0519−0593639 in their study.

References

Rahoui, F., Tomsick, J. A., Krivonos, R., 2017, MNRAS, 465, 2, 1563, 2017MNRAS.465.1563R

IGR J17164-3803