New Online Database of Symbiotic Variables: IPHAS J184144.00-012839.5

Constellation
Aquila

Equatorial coordinates
α = 18 41 44.003
δ = -01 28 39.575

Galactic coordinates
l = 30.5099°
b = 1.4843°

Suspected	2014^Ref
Confirmed	2014^Ref
Symbiotic IR type	S^Ref
Hot component type	shell-burning^Ref
Outbursts	-

Identifiers

IPHAS J184144.00-012839.5	IRAS -	GSC2.4.2 S9N7098959	AAVSO 000-BPJ-618
SIMBAD IPHAS J184144.00-012839.5	Pan-STARRS 106222804333477251	SAO -	VSX 2227403
GAIA DR3 4260144908078969344	SkyMapper 184144.00-012839.5	WRAY -	GCVS -
2MASS J18414400-0128394	HIP -	Hen -	BD -
WISE J184144.00-012839.4	TYC -	ESO -	HD -

Symbiotic Catalogs

Bidelman (1954)	-	Allen (1984)	-	Belzcyński et al. (2001)	-
Gaposchkin (1957)	-	Kenyon (1986)	-	Akras et al. (2019)	IPHASJ184144.00-012839.5 (Conf.)
Boyarchuk (1969)	-	Vaidis (1988, 1991)	-

Position

Right ascension (°)	280.4333^Ref	Parallax (mas)	0.067±0.138^Ref	Reddening E(B-V) (mag)	1.83±0.02^Ref ^{, Note}
Declination (°)	-1.4777^Ref	Distance (kpc)	7.6^Ref 5.61^Ref ^{, Note}, 4.45^Ref ^{, Note}
Galactic longitude (°)	30.5099^Ref	Proper motion in α (mas/yr)	-3.93±0.16^Ref
Galactic latitude (°)	1.4843^Ref	Proper motion in δ (mas/yr)	-6.00±0.14^Ref

Observations

X-Ray	-	IR type	S^Ref	Radio	-
X-Ray type	-	J (mag)	11.45^Ref	Flickering	-
GALEX FUV (mag)	-	H (mag)	9.99^Ref	Outbursts	-
GALEX NUV (mag)	-	K (mag)	9.33^Ref	Outburst type	-
IUE	No^Ref	WISE W1 (mag)	8.98^Ref	Jets	-
FUSE	No^Ref	WISE W2 (mag)	9.00^Ref	Resolved nebula	-
U (mag)	-	WISE W3 (mag)	8.65^Ref	IPmax (eV)	114^Ref
B (mag)	-	WISE W4 (mag)	8.45^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)	20.16^Ref	IRAS 100μm (Jy)	-
G (mag)	16.72^Ref	AKARI S09 (Jy)	-
RP (mag)	15.14^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	M5.6^Ref	Mass (M_⊙)	-	Pulsation	-
Eff. temperature (K)	3300^Ref	Radius (R_⊙)	-	Type	-
IR type	S^Ref	Luminosity (L_⊙)	915^Ref	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 symbiotic nature of the object is revealed by the strong TiO bands and the presence of high-excitation emission lines, including the prominent O VI Raman-scattered emission at 6825 Å (Rodríguez-Flores et al., 2014).

References

Rodríguez-Flores, E. R., Corradi, R. L. M., Mampaso, A. et al., 2014, A&A, 567, A49, 2014A&A...567A..49R

IPHAS J184144.00-012839.5