Hen 2-176

CONFIRMED MILKY WAY
 
Constellation
Scorpius
Equatorial coordinates
α = 16 41 31.202
δ = -45 13 04.716
Galactic coordinates
l = 339.3933°
b = 0.7448°

Suspected 1974Ref
Confirmed 1984Ref
Symbiotic IR type DRef, SRef
Hot component type shell-burningRef
Outbursts -

Identifiers

Hen 2-176 IRAS 16379-4507 GSC2.4.2 S8UV017816 AAVSO -
SIMBAD WRAY 16-230 Pan-STARRS - SAO - VSX 59169
GAIA DR3 5943382139466094720 SkyMapper 164131.19-451304.5 WRAY 16-230 GCVS -
2MASS J16413119-4513046 HIP - Hen 2-176 BD -
WISE J164131.15-451304.8 TYC - ESO 277-5 HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) He2-176 (Conf.) Belzcyński et al. (2001) Hen 2-176 (Conf.)
Gaposchkin (1957) - Kenyon (1986) He2-176 (Conf.) Akras et al. (2019) Hen 2-176 (Conf.)
Boyarchuk (1969) - Vaidis (1988, 1991) M-73 (Conf.)

Position

Right ascension (°) 250.3800Ref Parallax (mas) 0.043±0.092Ref Reddening E(B-V) (mag) 5.91±0.46Ref, Note
Declination (°) -45.2180Ref Distance (kpc) 2.6Ref
6.25Ref, Note, 4.05Ref, Note
   
Galactic longitude (°) 339.3933Ref Proper motion in α (mas/yr) -4.31±0.11Ref    
Galactic latitude (°) 0.7448Ref Proper motion in δ (mas/yr) -7.15±0.09Ref    

Observations

X-Ray NoRef IR type DRef, SRef Radio YesRef
X-Ray type - J (mag) 8.17Ref Flickering -
GALEX FUV (mag) - H (mag) 6.66Ref Outbursts -
GALEX NUV (mag) - K (mag) 5.78Ref Outburst type -
IUE NoRef WISE W1 (mag) 5.28Ref Jets -
FUSE NoRef WISE W2 (mag) 4.85Ref Resolved nebula NoRef
U (mag) - WISE W3 (mag) 4.23Ref IPmax (eV) 114Ref
B (mag) - WISE W4 (mag) 2.47Ref [O III] lines YesRef
V (mag) 15.00Ref IRAS 12μm (Jy) 2.81Ref He II lines YesRef
R (mag) - IRAS 25μm (Jy) 2.40Ref [Fe VII] lines YesRef
I (mag) - IRAS 60μm (Jy) 47.20Ref O VI lines YesRef
BP (mag) 16.08Ref IRAS 100μm (Jy) 289.00Ref
G (mag) 13.61Ref AKARI S09 (Jy) 1.09Ref
RP (mag) 11.96Ref AKARI S18 (Jy) 0.97Ref

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 M7 IIIRef, M4 IIIRef Mass (M) - Pulsation Yes?Ref
Eff. temperature (K) - Radius (R) - Type Mira?Ref
IR type DRef, 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) 4300Ref    
Lower limit (K) 114000Ref        
Upper limit (K) -        

Links

SIMBAD   CDS Portal


Notes

This stellar source, initially found with no emission lines in the blue by Webster (1966), has been subsequently observed with emission lines with ionization potential up to 114 eV by Allen (1984) and Stenholm & Acker (1987).


References


Last updated: April 17, 2022