GDS J1830235-135539

LIKELY MILKY WAY

Constellation
Scutum

Equatorial coordinates
α = 18 30 23.471
δ = -13 55 42.020

Galactic coordinates
l = 18.1623°
b = -1.7502°

Suspected	2022^Ref
Confirmed	-
Symbiotic IR type	D?^Ref
Hot component type	accreting-only?^Ref
Outbursts	Yes^Ref - SyN?^Ref

Identifiers

GDS J1830235-135539	IRAS 18275-1357	GSC2.4.2 S9JZ331839	AAVSO 000-BPL-326
SIMBAD IRAS 18275-1357	Pan-STARRS 91282775978046350	SAO -	VSX 456166
GAIA DR3 4104372315454847232	SkyMapper -	WRAY -	GCVS -
2MASS J18302347-1355421	HIP -	Hen -	BD -
WISE J183023.46-135541.9	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 (°)	277.5978^Ref	Parallax (mas)	-0.059±0.120^Ref	Reddening E(B-V) (mag)	1.77±0.03^Ref ^{, Note}
Declination (°)	-13.9283^Ref	Distance (kpc)	7.01^Ref ^{, Note}, 5.35^Ref ^{, Note}
Galactic longitude (°)	18.1623^Ref	Proper motion in α (mas/yr)	-4.47±0.13^Ref
Galactic latitude (°)	-1.7502^Ref	Proper motion in δ (mas/yr)	-8.78±0.10^Ref

Observations

X-Ray	-	IR type	D?^Ref	Radio	-
X-Ray type	-	J (mag)	8.28^Ref	Flickering	-
GALEX FUV (mag)	-	H (mag)	6.83^Ref	Outbursts	Yes^Ref
GALEX NUV (mag)	-	K (mag)	5.87^Ref	Outburst type	SyN?^Ref
IUE	No^Ref	WISE W1 (mag)	5.04^Ref	Jets	-
FUSE	No^Ref	WISE W2 (mag)	4.07^Ref	Resolved nebula	-
U (mag)	-	WISE W3 (mag)	3.09^Ref	IPmax (eV)	24.6^Ref
B (mag)	-	WISE W4 (mag)	2.14^Ref	[O III] lines	No^Ref
V (mag)	-	IRAS 12μm (Jy)	1.78^Ref	He II lines	No^Ref
R (mag)	-	IRAS 25μm (Jy)	1.11^Ref	[Fe VII] lines	No^Ref
I (mag)	12.13^Ref	IRAS 60μm (Jy)	22.30^Ref	O VI lines	No^Ref
BP (mag)	18.30^Ref	IRAS 100μm (Jy)	278.00^Ref
G (mag)	14.36^Ref	AKARI S09 (Jy)	2.47^Ref
RP (mag)	12.72^Ref	AKARI S18 (Jy)	1.26^Ref

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	-	Mass (M_⊙)	-	Pulsation	Yes^Ref
Eff. temperature (K)	-	Radius (R_⊙)	-	Type	Mira^Ref
IR type	D?^Ref	Luminosity (L_⊙)	-	Pulsation period (days)	315.3^Ref
Metallicity [Fe/H]	-			Pulsation ephemeris	-

Hot component

Type/Spectral type	-	Mass (M_⊙)	-	Spin period (min)	-
Shell-burning/Accreting-only	accreting-only?^Ref	Radius (R_⊙)	-	Accretion disk	-
Eff. temperature (K)	-	Luminosity (L_⊙)	-
Lower limit (K)	-
Upper limit (K)	-

Links

SIMBAD CDS Portal

Notes

Suggested to be a symbiotic nova with a Mira donor, according to Taguchi et al. (2022).

References

Taguchi, K., Yamamoto, M., Moriyama, M. et al., 2022, ATel, 15623, 1, 2022ATel15623....1T

Last updated: December 26, 2022