New Online Database of Symbiotic Variables: HV 13055

SUSPECTED LMC

Constellation
Dorado

Equatorial coordinates
α = 05 08 41.580
δ = -66 49 00.257

Galactic coordinates
l = 277.3274°
b = -34.8218°

Suspected	1970^Ref
Confirmed	-
Symbiotic IR type	S?^Ref
Hot component type	-
Outbursts	Yes?^Ref

Identifiers

HV 13055	IRAS -	GSC2.4.2 S1HJ096466	AAVSO -
SIMBAD SV* HV 13055	Pan-STARRS -	SAO -	VSX 2221187
GAIA DR3 4661952739447156608	SkyMapper 050841.57-664900.3	WRAY -	GCVS -
2MASS J05084158-6649004	HIP -	Hen -	BD -
WISE J050841.57-664900.1	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 (°)	77.1732^Ref	Parallax (mas)	-0.027±0.025^Ref	Reddening E(B-V) (mag)	0.17±0.01^Ref ^{, Note}
Declination (°)	-66.8167^Ref	Distance (kpc)	17.47^Ref ^{, Note}, 11.27^Ref ^{, Note}
Galactic longitude (°)	277.3274^Ref	Proper motion in α (mas/yr)	1.74±0.03^Ref
Galactic latitude (°)	-34.8218^Ref	Proper motion in δ (mas/yr)	0.22±0.03^Ref

Observations

X-Ray	-	IR type	S?^Ref	Radio	-
X-Ray type	-	J (mag)	13.34^Ref	Flickering	-
GALEX FUV (mag)	-	H (mag)	12.49^Ref	Outbursts	Yes?^Ref
GALEX NUV (mag)	-	K (mag)	12.24^Ref	Outburst type	-
IUE	No^Ref	WISE W1 (mag)	12.02^Ref	Jets	-
FUSE	No^Ref	WISE W2 (mag)	12.11^Ref	Resolved nebula	-
U (mag)	-	WISE W3 (mag)	11.68^Ref	IPmax (eV)	-
B (mag)	-	WISE W4 (mag)	9.04^Ref	[O III] lines	-
V (mag)	-	IRAS 12μm (Jy)	-	He II lines	-
R (mag)	-	IRAS 25μm (Jy)	-	[Fe VII] lines	-
I (mag)	-	IRAS 60μm (Jy)	-	O VI lines	-
BP (mag)	16.39^Ref	IRAS 100μm (Jy)	-
G (mag)	15.54^Ref	AKARI S09 (Jy)	-
RP (mag)	14.62^Ref	AKARI S18 (Jy)	-

Orbit

Orbital period (days)	682±90^Ref	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	-
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	-	Radius (R_⊙)	-	Accretion disk	-
Eff. temperature (K)	-	Luminosity (L_⊙)	-
Lower limit (K)	-
Upper limit (K)	-

Links

SIMBAD CDS Portal

Notes

The suggestion of a symbiotic nature for this star was made by Hodge & Wright (1970) due to light curve variations. However, this classification was rejected by Allen (1980) based on the observed low excitation in the spectrum. The star is also listed among RGB long-period variables in Spano et al. (2011).

References

Allen, D. A., 1980, ApL, 20, 131, 1980ApL....20..131A
Hodge, P. W., Wright, F. W., 1970, PASP, 82, 484, 135, 1970PASP...82..135H
Lindsay, E. M., 1971, IrAJ, 10, 141, 1971IrAJ...10..141L
Spano, M., Mowlavi, N., Eyer, L. et al., 2011, A&A, 536, A60, 2011A&A...536A..60S

HV 13055