New Online Database of Symbiotic Variables: StHA 190

Constellation
Aquarius

Equatorial coordinates
α = 21 41 44.892
δ = +02 43 54.479

Galactic coordinates
l = 58.4162°
b = -35.4321°

Suspected	1986^Ref
Confirmed	1988^Ref
Symbiotic IR type	D'^Ref
Hot component type	shell-burning^Ref
Outbursts	-

Identifiers

StHA 190	IRAS 21392+0230	GSC2.4.2 N0EP000242	AAVSO 000-BCY-230
SIMBAD EM* StHA 190	Pan-STARRS 111273254370338794	SAO -	VSX 64170
GAIA DR3 2694546586112887552	SkyMapper -	WRAY -	GCVS -
2MASS J21414488+0243543	HIP -	Hen -	BD -
WISE J214144.88+024354.3	TYC 547-712-1	ESO -	HD -

Symbiotic Catalogs

Bidelman (1954)	-	Allen (1984)	-	Belzcyński et al. (2001)	StHA 190 (Conf.)
Gaposchkin (1957)	-	Kenyon (1986)	-	Akras et al. (2019)	StHA 190 (Conf.)
Boyarchuk (1969)	-	Vaidis (1988, 1991)	-

Position

Right ascension (°)	325.4370^Ref	Parallax (mas)	0.878±0.020^Ref	Reddening E(B-V) (mag)	0.08±0.0^Ref ^{, Note}
Declination (°)	2.7318^Ref	Distance (kpc)	1.10^Ref ^{, Note}, 1.08^Ref ^{, Note}
Galactic longitude (°)	58.4162^Ref	Proper motion in α (mas/yr)	3.86±0.02^Ref
Galactic latitude (°)	-35.4321^Ref	Proper motion in δ (mas/yr)	4.04±0.01^Ref

Observations

X-Ray	No^Ref, No^Ref, Yes^Ref	IR type	D'^Ref	Radio	Yes^Ref
X-Ray type	β^Ref	J (mag)	8.71^Ref	Flickering	No^Ref
GALEX FUV (mag)	-	H (mag)	8.21^Ref	Outbursts	-
GALEX NUV (mag)	-	K (mag)	8.02^Ref	Outburst type	-
IUE	Yes^Ref	WISE W1 (mag)	7.78^Ref	Jets	Yes^Ref
FUSE	No^Ref	WISE W2 (mag)	7.44^Ref	Resolved nebula	-
U (mag)	-	WISE W3 (mag)	4.12^Ref	IPmax (eV)	35.1^Ref
B (mag)	11.40^Ref	WISE W4 (mag)	2.13^Ref	[O III] lines	Yes^Ref
V (mag)	10.54^Ref	IRAS 12μm (Jy)	1.84^Ref	He II lines	No^Ref
R (mag)	-	IRAS 25μm (Jy)	1.65^Ref	[Fe VII] lines	No^Ref
I (mag)	-	IRAS 60μm (Jy)	0.40^Ref	O VI lines	No^Ref
BP (mag)	10.73^Ref	IRAS 100μm (Jy)	2.95^Ref
G (mag)	10.26^Ref	AKARI S09 (Jy)	0.85^Ref
RP (mag)	9.60^Ref	AKARI S18 (Jy)	1.06^Ref

Orbit

Orbital period (days)	171±7^Ref	γ velocity (km/h)	-3.18±2.37^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	G5 III^Ref	Mass (M_⊙)	2.5^Ref, 2.25^Ref	Pulsation	-
Eff. temperature (K)	5150^Ref, 5300±150^Ref	Radius (R_⊙)	8.3^Ref, 7.88^Ref	Type	-
IR type	D'^Ref	Luminosity (L_⊙)	45^Ref	Pulsation period (days)	-
Metallicity [Fe/H]	0^Ref			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)	-
Upper limit (K)	-

Links

SIMBAD CDS Portal ARAS Database

Notes

Initially classified as a probable symbiotic star by Stephenson (1986), who noted a very red continuum together with emission lines. The symbiotic nature was subsequently confirmed by observations in Downes & Keyes (1988). In Munari et al. (2001), the discovery of a bipolar and highly variable mass outflow from the system was reported. They also claimed that the system has a very short orbital period of 171 days. The cool component in the system was identified as an extremely fast rotator in Zamanov et al. (2006).

References

Downes, R. A., Keyes, C. D., 1988, AJ, 96, 777, 1988AJ.....96..777D
Merc, J., Beck, P. G., Mathur, S. et al., 2023, arXiv, arXiv:2312.16126, 2023arXiv231216126M
Munari, U., Tomov, T., Yudin, B. F. et al., 2001, A&A, 369, L1, 2001A&A...369L...1M
Mürset, U., Schmid, H. M., 1999, A&AS, 137, 473, 1999A&AS..137..473M
Schmid, H. M., Nussbaumer, H., 1993, A&A, 268, 159, 1993A&A...268..159S
Smith, V. V., Pereira, C. B., Cunha, K., 2001, ApJL, 556, 1, L55, 2001ApJ...556L..55S
Sokoloski, J. L., Bildsten, L., Ho, W. C. G., 2001, MNRAS, 326, 2, 553, 2001MNRAS.326..553S
Stephenson, C. B., 1986, ApJ, 300, 779, 1986ApJ...300..779S
Zamanov, R. K., Bode, M. F., Melo, C. H. F. et al., 2006, MNRAS, 365, 4, 1215, 2006MNRAS.365.1215Z

StHA 190