PN H1-43

MISCLASSIFIED MILKY WAY
 
Constellation
Scorpius
Equatorial coordinates
α = 17 58 14.438
δ = -33 47 37.716
Galactic coordinates
l = 357.1835°
b = -4.7886°

Suspected 1974Ref
Re-classified 1992Ref
Type PN with WR central starRef

Identifiers

PN H1-43 IRAS 17549-3347 GSC2.4.2 S8GW040360 AAVSO -
SIMBAD PN H 1-43 Pan-STARRS - SAO - VSX -
GAIA DR3 4042380857826322176 SkyMapper - WRAY 16-335 GCVS -
2MASS J17581444-3347375 HIP - Hen 2-313 BD -
WISE - TYC - ESO 394-15 HD -

Symbiotic Catalogs

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

Position

Right ascension (°) 269.5602Ref Parallax (mas) 0.571±0.061Ref Reddening E(B-V) (mag) 0.57±0.04Ref, Note
Declination (°) -33.7938Ref Distance (kpc) 1.66Ref, Note, 1.70Ref, Note    
Galactic longitude (°) 357.1835Ref Proper motion in α (mas/yr) -1.39±0.07Ref    
Galactic latitude (°) -4.7886Ref Proper motion in δ (mas/yr) -5.90±0.04Ref    

Links

SIMBAD   CDS Portal


Notes

In 1974, based on infrared photometry, it was suggested by Allen & Glass (1974) that this southern planetary nebula exhibits a continuum similar to that of symbiotic and VV Cephei stars. In Acker et al. (1992), the target is classified as a true PN.


References

  • Acker, A., Marcout, J., Ochsenbein, F. et al., 1992, The Strasbourg-ESO Catalogue of Galactic Planetary Nebulae. Parts I, 1, 1992secg.book.....A
  • Allen, D. A., Glass, I. S., 1974, MNRAS, 167, 337, 1974MNRAS.167..337A


Last updated: April 30, 2022