Hen 2-251

CONFIRMED MILKY WAY
 
Constellation
Ophiucus
Equatorial coordinates
α = 17 35 22.232
δ = -29 45 19.894
Galactic coordinates
l = 358.1205°
b = 1.4588°

Suspected 1987Ref
Confirmed 1987Ref
Symbiotic IR type DRef
Hot component type shell-burningRef
Outbursts -

Identifiers

Hen 2-251 IRAS 17321-2943 GSC2.4.2 S8H0265936 AAVSO 000-BLC-802
SIMBAD PN H 1-25 Pan-STARRS 72292638426293651 SAO - VSX 61207
GAIA DR3 4058561820720486272 SkyMapper 173522.23-294519.6 WRAY 16-289 GCVS -
2MASS J17352223-2945198 HIP - Hen 2-251 BD -
WISE J173522.22-294519.7 TYC - ESO 455-22 HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) - Belzcyński et al. (2001) Hen 2-251 (Conf.)
Gaposchkin (1957) - Kenyon (1986) - Akras et al. (2019) Hen 2-251 (Conf.)
Boyarchuk (1969) - Vaidis (1988, 1991) H-1-25 (Susp.)

Position

Right ascension (°) 263.8426Ref Parallax (mas) 0.043±0.075Ref Reddening E(B-V) (mag) 2.15±0.13Ref, Note
Declination (°) -29.7555Ref Distance (kpc) 8.5Ref
8.86Ref, Note, 5.74Ref, Note
   
Galactic longitude (°) 358.1205Ref Proper motion in α (mas/yr) -6.03±0.09Ref    
Galactic latitude (°) 1.4588Ref Proper motion in δ (mas/yr) 0.87±0.06Ref    

Observations

X-Ray NoRef IR type DRef Radio NoRef
X-Ray type - J (mag) 10.42Ref Flickering -
GALEX FUV (mag) - H (mag) 8.63Ref Outbursts -
GALEX NUV (mag) - K (mag) 6.95Ref Outburst type -
IUE NoRef WISE W1 (mag) 4.63Ref Jets -
FUSE NoRef WISE W2 (mag) 3.61Ref Resolved nebula -
U (mag) - WISE W3 (mag) 1.72Ref IPmax (eV) 114Ref
B (mag) - WISE W4 (mag) 0.30Ref [O III] lines YesRef
V (mag) 15.70Ref IRAS 12μm (Jy) 7.33Ref He II lines YesRef
R (mag) - IRAS 25μm (Jy) 7.46Ref [Fe VII] lines YesRef
I (mag) - IRAS 60μm (Jy) 2.54Ref O VI lines YesRef
BP (mag) 16.87Ref IRAS 100μm (Jy) 75.30Ref
G (mag) 15.81Ref AKARI S09 (Jy) -
RP (mag) 14.59Ref AKARI S18 (Jy) 5.69Ref

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 K5Ref, late MRef Mass (M) - Pulsation -
Eff. temperature (K) - Radius (R) - Type -
IR type DRef 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) 5700Ref    
Lower limit (K) 114000Ref        
Upper limit (K) -        

Links

SIMBAD   CDS Portal


Notes

Initially suspected in Acker et al. (1992), the symbiotic nature of this star was confirmed by the detection of strong O VI lines by Stenholm & Acker (1987) and Cieslinski et al. (1994).


References

  • Acker, A., Marcout, J., Ochsenbein, F. et al., 1992, The Strasbourg-ESO Catalogue of Galactic Planetary Nebulae. Parts I, 1, 1992secg.book.....A
  • Cieslinski, D., Elizalde, F., Steiner, J. E., 1994, A&AS, 106, 243, 1994A&AS..106..243C
  • Mikołajewska, J., Acker, A., Stenholm, B., 1997, A&A, 327, 191, 1997A&A...327..191M
  • Stenholm, B., Acker, A., 1987, A&AS, 68, 51, 1987A&AS...68...51S


Last updated: April 14, 2022