MISCLASSIFIED
    MILKY WAY
 
  | 
    
| M 4-12 | IRAS 19108+1541 | GSC2.4.2 N2CY173813 | AAVSO 000-BKR-766 | 
| SIMBAD PN M 4-12 | Pan-STARRS 126932882727173793 | SAO - | VSX 249541 | 
| GAIA DR3 4513170261953875840 | SkyMapper - | WRAY - | GCVS - | 
| 2MASS J19130545+1546399 | HIP - | Hen 2-428 | BD - | 
| WISE J191305.45+154639.8 | TYC - | ESO - | HD - | 
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - | 
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - | 
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | - | 
| Right ascension (°) | 288.2727Ref | Parallax (mas) | 0.224±0.075Ref | Reddening E(B-V) (mag) | 1.69±0.13Ref, Note | 
| Declination (°) | 15.7777Ref | Distance (kpc) | 4.08Ref, Note, 3.27Ref, Note | ||
| Galactic longitude (°) | 49.4103Ref | Proper motion in α (mas/yr) | -2.17±0.07Ref | ||
| Galactic latitude (°) | 2.4753Ref | Proper motion in δ (mas/yr) | -12.55±0.06Ref | 
The suspicion of being a symbiotic star for this object was raised by Rodríguez et al. (2001) due to the presence of an aged, extended nebula with a dense nebular core. Subsequently, in 2015, the discovery of a double degenerate core with a combined mass exceeding the Chandrasekhar limit was reported (Santander-García et al., 2015).