New Online Database of Symbiotic Variables: IPHAS J190441.53-005957.2

Constellation
Aquila

Equatorial coordinates
α = 19 04 41.532
δ = -00 59 57.240

Galactic coordinates
l = 33.5536°
b = -3.4046°

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

Identifiers

IPHAS J190441.53-005957.2	IRAS 19021-0103	GSC2.4.2 S9MG019204	AAVSO -
SIMBAD IPHAS J190441.53-005957.2	Pan-STARRS 106802861730821370	SAO -	VSX 238545
GAIA DR3 4262488139186420480	SkyMapper 190441.52-005957.0	WRAY -	GCVS -
2MASS J19044153-0059571	HIP -	Hen -	BD -
WISE J190441.53-005957.1	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 (°)	286.1731^Ref	Parallax (mas)	-0.229±0.097^Ref	Reddening E(B-V) (mag)	0.72±0.03^Ref ^{, Note}
Declination (°)	-0.9992^Ref	Distance (kpc)	8.99^Ref ^{, Note}, 7.45^Ref ^{, Note}
Galactic longitude (°)	33.5536^Ref	Proper motion in α (mas/yr)	-2.44±0.11^Ref
Galactic latitude (°)	-3.4046^Ref	Proper motion in δ (mas/yr)	-4.90±0.09^Ref

Observations

X-Ray	-	IR type	D?^Ref	Radio	-
X-Ray type	-	J (mag)	8.89^Ref	Flickering	-
GALEX FUV (mag)	-	H (mag)	7.75^Ref	Outbursts	-
GALEX NUV (mag)	-	K (mag)	7.17^Ref	Outburst type	-
IUE	No^Ref	WISE W1 (mag)	6.68^Ref	Jets	-
FUSE	No^Ref	WISE W2 (mag)	6.66^Ref	Resolved nebula	-
U (mag)	-	WISE W3 (mag)	5.97^Ref	IPmax (eV)	-
B (mag)	-	WISE W4 (mag)	5.55^Ref	[O III] lines	-
V (mag)	-	IRAS 12μm (Jy)	1.02^Ref	He II lines	-
R (mag)	-	IRAS 25μm (Jy)	0.38^Ref	[Fe VII] lines	-
I (mag)	-	IRAS 60μm (Jy)	0.97^Ref	O VI lines	-
BP (mag)	18.13^Ref	IRAS 100μm (Jy)	75.90^Ref
G (mag)	14.54^Ref	AKARI S09 (Jy)	0.19^Ref
RP (mag)	12.95^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	M6.8^Ref	Mass (M_⊙)	-	Pulsation	-
Eff. temperature (K)	-	Radius (R_⊙)	-	Type	-
IR type	D?^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

The object exhibits a red giant continuum and an emission line spectrum. However, the observed emission lines are all of low ionization (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 J190441.53-005957.2