New Online Database of Symbiotic Variables: [MMU2013] 356.04+03.20

Constellation
Scorpius

Equatorial coordinates
α = 17 23 21.278
δ = -30 31 36.054

Galactic coordinates
l = 356.0429°
b = 3.2005°

Suspected	2013^Ref
Confirmed	2013^Ref
Symbiotic IR type	S^Ref
Hot component type	shell-burning^Ref
Outbursts	-

Identifiers

[MMU2013] 356.04+03.20	IRAS -	GSC2.4.2 S8HO087893	AAVSO -
SIMBAD 2MASS J17232128-3031358	Pan-STARRS 71362608386598308	SAO -	VSX 305981
GAIA DR3 4059014991298469248	SkyMapper 172321.27-303136.0	WRAY -	GCVS -
2MASS J17232128-3031358	HIP -	Hen -	BD -
WISE J172321.30-303136.3	TYC -	ESO -	HD -

Symbiotic Catalogs

Bidelman (1954)	-	Allen (1984)	-	Belzcyński et al. (2001)	-
Gaposchkin (1957)	-	Kenyon (1986)	-	Akras et al. (2019)	356.04+03.20 (Conf.)
Boyarchuk (1969)	-	Vaidis (1988, 1991)	-

Position

Right ascension (°)	260.8387^Ref	Parallax (mas)	0.028±0.086^Ref	Reddening E(B-V) (mag)	1.72±0.11^Ref ^{, Note}
Declination (°)	-30.5267^Ref	Distance (kpc)	7.40^Ref ^{, Note}, 6.60^Ref ^{, Note}
Galactic longitude (°)	356.0429^Ref	Proper motion in α (mas/yr)	-2.46±0.10^Ref
Galactic latitude (°)	3.2005^Ref	Proper motion in δ (mas/yr)	-6.66±0.07^Ref

Observations

X-Ray	-	IR type	S^Ref	Radio	-
X-Ray type	-	J (mag)	9.79^Ref	Flickering	-
GALEX FUV (mag)	-	H (mag)	8.46^Ref	Outbursts	-
GALEX NUV (mag)	-	K (mag)	7.87^Ref	Outburst type	-
IUE	No^Ref	WISE W1 (mag)	7.24^Ref	Jets	-
FUSE	No^Ref	WISE W2 (mag)	7.61^Ref	Resolved nebula	-
U (mag)	-	WISE W3 (mag)	7.21^Ref	IPmax (eV)	114^Ref
B (mag)	-	WISE W4 (mag)	6.58^Ref	[O III] lines	No^Ref
V (mag)	-	IRAS 12μm (Jy)	-	He II lines	Yes^Ref
R (mag)	-	IRAS 25μm (Jy)	-	[Fe VII] lines	Yes^Ref
I (mag)	-	IRAS 60μm (Jy)	-	O VI lines	Yes^Ref
BP (mag)	18.21^Ref	IRAS 100μm (Jy)	-
G (mag)	14.78^Ref	AKARI S09 (Jy)	-
RP (mag)	13.22^Ref	AKARI S18 (Jy)	-

Orbit

Orbital period (days)	-	γ velocity (km/h)	0.42±2.54^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	M6^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	shell-burning^Ref	Radius (R_⊙)	-	Accretion disk	-
Eff. temperature (K)	-	Luminosity (L_⊙)	-
Lower limit (K)	114000^Ref
Upper limit (K)	-

Links

SIMBAD CDS Portal

Notes

The emission-line spectrum of this star is in accordance with that of a highly ionized S-type symbiotic, as reported in Miszalski et al. (2013). The weak but detected Raman-scattered O VI 6825 feature aligns with the presence of [Fe VII] emission in the spectrum.

References

Miszalski, B., Mikołajewska, J., Udalski, A., 2013, MNRAS, 432, 4, 3186, 2013MNRAS.432.3186M

[MMU2013] 356.04+03.20