Th 3-18

CONFIRMED MILKY WAY
 
Constellation
Ophiucus
Equatorial coordinates
α = 17 28 26.924
δ = -28 38 34.717
Galactic coordinates
l = 358.2276°
b = 3.3318°

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

Identifiers

Th 3-18 IRAS - GSC2.4.2 S8G8039602 AAVSO 000-BJT-834
SIMBAD PN Th 3-18 Pan-STARRS 73622621122188720 SAO - VSX 241041
GAIA DR3 4059655594297061888 SkyMapper 172826.93-283834.5 WRAY 17-83 GCVS -
2MASS J17282693-2838345 HIP - Hen 2-228 BD -
WISE J172826.93-283834.6 TYC - ESO 454-32 HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) Th3-18 (Conf.) Belzcyński et al. (2001) Th 3-18 (Conf.)
Gaposchkin (1957) - Kenyon (1986) Th3-18 (Conf.) Akras et al. (2019) PN Th 3-18 (Conf.)
Boyarchuk (1969) - Vaidis (1988, 1991) Th-3-18 (Conf.)

Position

Right ascension (°) 262.1122Ref Parallax (mas) 0.152±0.040Ref Reddening E(B-V) (mag) 1.14±0.02Ref, Note
Declination (°) -28.6430Ref Distance (kpc) 3.5Ref, 4.2Ref
5.07Ref, Note, 4.75Ref, Note
   
Galactic longitude (°) 358.2276Ref Proper motion in α (mas/yr) -4.04±0.05Ref    
Galactic latitude (°) 3.3318Ref Proper motion in δ (mas/yr) -4.97±0.04Ref    

Observations

X-Ray NoRef IR type SRef Radio NoRef
X-Ray type - J (mag) 9.82Ref Flickering -
GALEX FUV (mag) - H (mag) 8.67Ref Outbursts -
GALEX NUV (mag) - K (mag) 8.23Ref Outburst type -
IUE NoRef WISE W1 (mag) 8.01Ref Jets -
FUSE NoRef WISE W2 (mag) 7.98Ref Resolved nebula -
U (mag) - WISE W3 (mag) 7.71Ref IPmax (eV) 114Ref
B (mag) - WISE W4 (mag) 7.10Ref [O III] lines Yes?Ref
V (mag) 15.30Ref IRAS 12μm (Jy) - He II lines YesRef
R (mag) 15.44Ref IRAS 25μm (Jy) - [Fe VII] lines NoRef
I (mag) - IRAS 60μm (Jy) - O VI lines YesRef
BP (mag) 16.15Ref IRAS 100μm (Jy) -
G (mag) 13.91Ref AKARI S09 (Jy) -
RP (mag) 12.53Ref AKARI S18 (Jy) -

Orbit

Orbital period (days) - γ velocity (km/h) 122.84±0.68Ref 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 M2 IIIRef, M3 IIIRef,
M2 IIIRef
Mass (M) - Pulsation -
Eff. temperature (K) 3649Ref 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) 750Ref    
Lower limit (K) 114000Ref        
Upper limit (K) -        

Links

SIMBAD   CDS Portal


Notes

Allen (1984) and Stenholm & Acker (1987) detected emission lines with ionization potential up to 114 eV.


References


Last updated: April 17, 2022