New Online Database of Symbiotic Variables: Pt 1

Constellation
Ophiucus

Equatorial coordinates
α = 17 38 49.546
δ = -23 54 04.148

Galactic coordinates
l = 3.4833°
b = 3.9422°

Suspected	1980^Ref
Confirmed	1980^Ref
Symbiotic IR type	S^Ref
Hot component type	shell-burning^Ref
Outbursts	-

Identifiers

Pt 1	IRAS -	GSC2.4.2 S8CK027594	AAVSO -
SIMBAD ESO 520-12	Pan-STARRS 79312647064348091	SAO -	VSX -
GAIA DR3 4116352873442484096	SkyMapper 173849.53-235406.6	WRAY -	GCVS -
2MASS J17384954-2354066	HIP -	Hen -	BD -
WISE J173849.54-235406.6	TYC -	ESO -	HD -

Symbiotic Catalogs

Bidelman (1954)	-	Allen (1984)	Pt-1 (Conf.)	Belzcyński et al. (2001)	Pt 1 (Conf.)
Gaposchkin (1957)	-	Kenyon (1986)	Pt-1 (Conf.)	Akras et al. (2019)	PN Pt 1 (Conf.)
Boyarchuk (1969)	-	Vaidis (1988, 1991)	NSV 9354 (Conf.)

Position

Right ascension (°)	264.7064^Ref	Parallax (mas)	0.103±0.022^Ref	Reddening E(B-V) (mag)	0.83±0.01^Ref ^{, Note}
Declination (°)	-23.9019^Ref	Distance (kpc)	2.7^Ref 6.44^Ref ^{, Note}, 5.66^Ref ^{, Note}
Galactic longitude (°)	3.4833^Ref	Proper motion in α (mas/yr)	-0.16±0.03^Ref
Galactic latitude (°)	3.9422^Ref	Proper motion in δ (mas/yr)	-10.19±0.01^Ref

Observations

X-Ray	No^Ref	IR type	S^Ref	Radio	No^Ref
X-Ray type	-	J (mag)	10.09^Ref	Flickering	-
GALEX FUV (mag)	-	H (mag)	8.91^Ref	Outbursts	-
GALEX NUV (mag)	-	K (mag)	8.49^Ref	Outburst type	-
IUE	No^Ref	WISE W1 (mag)	8.24^Ref	Jets	-
FUSE	No^Ref	WISE W2 (mag)	8.21^Ref	Resolved nebula	-
U (mag)	-	WISE W3 (mag)	7.86^Ref	IPmax (eV)	114^Ref
B (mag)	17.27^Ref	WISE W4 (mag)	7.16^Ref	[O III] lines	No?^Ref
V (mag)	15.46^Ref	IRAS 12μm (Jy)	-	He II lines	Yes^Ref
R (mag)	-	IRAS 25μm (Jy)	-	[Fe VII] lines	No^Ref
I (mag)	-	IRAS 60μm (Jy)	-	O VI lines	Yes^Ref
BP (mag)	15.71^Ref	IRAS 100μm (Jy)	-
G (mag)	13.83^Ref	AKARI S09 (Jy)	-
RP (mag)	12.54^Ref	AKARI S18 (Jy)	-

Orbit

Orbital period (days)	-	γ velocity (km/h)	-350.00±10.00^Ref	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	M1^Ref, M0 III^Ref, M3 III^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_⊙)	0.15^Ref	Accretion disk	-
Eff. temperature (K)	125000^Ref	Luminosity (L_⊙)	-
Lower limit (K)	-
Upper limit (K)	-

Links

SIMBAD CDS Portal

Notes

In Peterson (1977), the star was associated with the globular cluster NGC 6401. However, this association was later rejected by Munari et al. (1994), who argued that the symbiotic star is a halo object.

References

Allen, D. A., 1984, PASA, 5, 3, 369, 1984PASA....5..369A
Munari, U., Lattanzi, M. G., Bragaglia, A., 1994, A&A, 292, 501, 1994A&A...292..501M
Peterson, A. W., 1977, PASP, 89, 129, 1977PASP...89..129P
Torres-Peimbert, S., Recillas-Cruz, E., Peimbert, M., 1980, RMxAA, 5, 51, 1980RMxAA...5...51T

Pt 1