Th 3-30

CONFIRMED MILKY WAY
 
Constellation
Ophiucus
Equatorial coordinates
α = 17 33 43.387
δ = -28 07 21.189
Galactic coordinates
l = 359.2995°
b = 2.6456°

Suspected 1979Ref
Confirmed 1984Ref
Symbiotic IR type SRef
Hot component type shell-burningRef
Outbursts -

Identifiers

Th 3-30 IRAS - GSC2.4.2 S8DS058514 AAVSO 000-BJT-836
SIMBAD PN Th 3-30 Pan-STARRS 74252634308063244 SAO - VSX 241045
GAIA DR3 4061159206381600000 SkyMapper 173343.39-280721.4 WRAY 17-90 GCVS -
2MASS J17334338-2807211 HIP - Hen - BD -
WISE J173343.39-280721.2 TYC - ESO - HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) Th3-30 (Conf.) Belzcyński et al. (2001) Th 3-30 (Conf.)
Gaposchkin (1957) - Kenyon (1986) Th3-30 (Conf.) Akras et al. (2019) PN Th 3-30 (Conf.)
Boyarchuk (1969) - Vaidis (1988, 1991) Th-3-30 (Conf.)

Position

Right ascension (°) 263.4308Ref Parallax (mas) 0.001±0.052Ref Reddening E(B-V) (mag) 1.33±0.02Ref, Note
Declination (°) -28.1226Ref Distance (kpc) 3.8Ref
8.92Ref, Note, 6.45Ref, Note
   
Galactic longitude (°) 359.2995Ref Proper motion in α (mas/yr) 3.24±0.05Ref    
Galactic latitude (°) 2.6456Ref Proper motion in δ (mas/yr) -7.26±0.03Ref    

Observations

X-Ray NoRef IR type SRef Radio NoRef
X-Ray type - J (mag) 10.17Ref Flickering -
GALEX FUV (mag) - H (mag) 8.86Ref Outbursts -
GALEX NUV (mag) - K (mag) 8.33Ref Outburst type -
IUE NoRef WISE W1 (mag) 7.94Ref Jets -
FUSE NoRef WISE W2 (mag) 7.90Ref Resolved nebula -
U (mag) - WISE W3 (mag) 7.43Ref IPmax (eV) 114Ref
B (mag) - WISE W4 (mag) 6.66Ref [O III] lines NoRef
V (mag) 16.10Ref IRAS 12μm (Jy) - He II lines YesRef
R (mag) - IRAS 25μm (Jy) - [Fe VII] lines NoRef
I (mag) - IRAS 60μm (Jy) - O VI lines YesRef
BP (mag) 16.49Ref IRAS 100μm (Jy) -
G (mag) 14.30Ref AKARI S09 (Jy) -
RP (mag) 12.91Ref AKARI S18 (Jy) -

Orbit

Orbital period (days) - γ velocity (km/h) -13.09±4.95Ref 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 K5 IIIRef, K5 IIIRef,
M1 IIIRef
Mass (M) - Pulsation -
Eff. temperature (K) 3976Ref Radius (R) - Type -
IR type SRef Luminosity (L) - Pulsation period (days) -
Metallicity [Fe/H] -     Pulsation ephemeris -

Hot component

Type/Spectral type WDRef Mass (M) - Spin period (min) -
Shell-burning/Accreting-only shell-burningRef Radius (R) - Accretion disk -
Eff. temperature (K) - Luminosity (L) 100Ref    
Lower limit (K) 114000Ref        
Upper limit (K) -        

Links

SIMBAD   CDS Portal


Notes

In Stenholm & Acker (1987), the detection of strong O VI lines was reported for this object.


References


Last updated: April 17, 2022