New Online Database of Symbiotic Variables: IPHAS J185323.58+084955.1

Constellation
Aquila

Equatorial coordinates
α = 18 53 23.582
δ = +08 49 55.006

Galactic coordinates
l = 41.0240°
b = 3.5838°

Suspected	2010^Ref
Confirmed	2010^Ref
Symbiotic IR type	S^Ref
Hot component type	shell-burning^Ref
Outbursts	-

Identifiers

IPHAS J185323.58+084955.1	IRAS -	GSC2.4.2 N1N6006550	AAVSO 000-BKT-293
SIMBAD IPHAS J185323.58+084955.1	Pan-STARRS 118592833482608852	SAO -	VSX 238537
GAIA DR3 4310363383682200960	SkyMapper -	WRAY -	GCVS -
2MASS J18532358+0849551	HIP -	Hen -	BD -
WISE J185323.58+084955.0	TYC -	ESO -	HD -

Symbiotic Catalogs

Bidelman (1954)	-	Allen (1984)	-	Belzcyński et al. (2001)	-
Gaposchkin (1957)	-	Kenyon (1986)	-	Akras et al. (2019)	IPHASJ185323.58+084955.0 (Conf.)
Boyarchuk (1969)	-	Vaidis (1988, 1991)	-

Position

Right ascension (°)	283.3483^Ref	Parallax (mas)	0.066±0.068^Ref	Reddening E(B-V) (mag)	1.37±0.03^Ref ^{, Note}
Declination (°)	8.8319^Ref	Distance (kpc)	6.5^Ref 6.75^Ref ^{, Note}, 5.11^Ref ^{, Note}
Galactic longitude (°)	41.0240^Ref	Proper motion in α (mas/yr)	-1.96±0.07^Ref
Galactic latitude (°)	3.5838^Ref	Proper motion in δ (mas/yr)	-6.05±0.08^Ref

Observations

X-Ray	-	IR type	S^Ref	Radio	-
X-Ray type	-	J (mag)	10.32^Ref	Flickering	-
GALEX FUV (mag)	-	H (mag)	9.05^Ref	Outbursts	-
GALEX NUV (mag)	-	K (mag)	8.52^Ref	Outburst type	-
IUE	No^Ref	WISE W1 (mag)	8.19^Ref	Jets	-
FUSE	No^Ref	WISE W2 (mag)	8.18^Ref	Resolved nebula	-
U (mag)	-	WISE W3 (mag)	7.70^Ref	IPmax (eV)	114^Ref
B (mag)	-	WISE W4 (mag)	7.00^Ref	[O III] lines	Yes^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)	18.08^Ref	IRAS 100μm (Jy)	-
G (mag)	15.36^Ref	AKARI S09 (Jy)	-
RP (mag)	13.84^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	M6.5^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)	-
Upper limit (K)	-

Links

SIMBAD CDS Portal

Notes

Displaying a classical spectrum of a symbiotic star, the object exhibits a prominent continuum with TiO bands in the red part of the spectrum and an emission line spectrum (Corradi et al., 2010).

References

Corradi, R. L. M., Valentini, M., Munari, U. et al., 2010, A&A, 509, A41, 2010A&A...509A..41C

IPHAS J185323.58+084955.1