New Online Database of Symbiotic Variables: IGR J17197-3010

Constellation
Ophiucus

Equatorial coordinates
α = 17 19 51.825
δ = -30 02 00.687

Galactic coordinates
l = 356.0225°
b = 4.1009°

Suspected	2012^Ref
Confirmed	2013^Ref
Symbiotic IR type	S^Ref
Hot component type	accreting-only?^Ref
Outbursts	-

Identifiers

IGR J17197-3010	IRAS -	GSC2.4.2 S8HO121332	AAVSO 000-BLH-190
SIMBAD UCAC4 300-127036	Pan-STARRS 71962599659790183	SAO -	VSX 358659
GAIA DR3 4059196651237110272	SkyMapper 171951.84-300200.7	WRAY -	GCVS -
2MASS J17195182-3002003	HIP -	Hen -	BD -
WISE J171951.86-300201.2	TYC -	ESO -	HD -

Symbiotic Catalogs

Bidelman (1954)	-	Allen (1984)	-	Belzcyński et al. (2001)	-
Gaposchkin (1957)	-	Kenyon (1986)	-	Akras et al. (2019)	SWIFTJ171951.7-300206 (Conf.)
Boyarchuk (1969)	-	Vaidis (1988, 1991)	-

Position

Right ascension (°)	259.9659^Ref	Parallax (mas)	5.291±0.021^Ref	Reddening E(B-V) (mag)	0.9±0.02^Ref ^{, Note}
Declination (°)	-30.0335^Ref	Distance (kpc)	6.3^Ref 0.19^Ref ^{, Note}, 0.19^Ref ^{, Note}
Galactic longitude (°)	356.0225^Ref	Proper motion in α (mas/yr)	-0.76±0.02^Ref
Galactic latitude (°)	4.1009^Ref	Proper motion in δ (mas/yr)	-21.16±0.02^Ref

Observations

X-Ray	Yes^Ref	IR type	S^Ref	Radio	-
X-Ray type	β^Ref	J (mag)	10.88^Ref	Flickering	-
GALEX FUV (mag)	-	H (mag)	10.19^Ref	Outbursts	-
GALEX NUV (mag)	-	K (mag)	9.97^Ref	Outburst type	-
IUE	No^Ref	WISE W1 (mag)	9.58^Ref	Jets	-
FUSE	No^Ref	WISE W2 (mag)	9.53^Ref	Resolved nebula	-
U (mag)	-	WISE W3 (mag)	9.45^Ref	IPmax (eV)	-
B (mag)	-	WISE W4 (mag)	8.23^Ref	[O III] lines	-
V (mag)	-	IRAS 12μm (Jy)	-	He II lines	-
R (mag)	-	IRAS 25μm (Jy)	-	[Fe VII] lines	-
I (mag)	-	IRAS 60μm (Jy)	-	O VI lines	-
BP (mag)	15.08^Ref	IRAS 100μm (Jy)	-
G (mag)	13.74^Ref	AKARI S09 (Jy)	-
RP (mag)	12.58^Ref	AKARI S18 (Jy)	-

Orbit

Orbital period (days)	-	γ velocity (km/h)	36.66±7.20^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	M1-2^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 by Masetti et al. (2012) with a potential M giant counterpart, this object's symbiotic classification was later confirmed by Luna et al. (2013) based on X-ray data from Swift. However, they contested the proposal from Masetti et al. (2012) that this object is a counterpart of the γ-ray source.

References

Luna, G. J. M., Sokoloski, J. L., Mukai, K. et al., 2013, A&A, 559, A6, 2013A&A...559A...6L
Masetti, N., Parisi, P., Jiménez-Bailón, E. et al., 2012, A&A, 538, A123, 2012A&A...538A.123M

IGR J17197-3010