MISCLASSIFIED
MILKY WAY
|
| HD 169226 | IRAS - | GSC2.4.2 S9JO092667 | AAVSO - |
| SIMBAD HD 169226 | Pan-STARRS 93342760491063505 | SAO 161431 | VSX 62860 |
| GAIA DR3 4153236162693785856 | SkyMapper - | WRAY - | GCVS - |
| 2MASS J18241176-1212505 | HIP - | Hen - | BD -12 5034 |
| WISE J182411.75-121250.3 | TYC 5698-5323-1 | ESO - | HD 169226 |
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
| Right ascension (°) | 276.0490Ref | Parallax (mas) | 0.486±0.028Ref | Reddening E(B-V) (mag) | 5.09±0.67Ref, Note |
| Declination (°) | -12.2140Ref | Distance (kpc) | 1.90Ref, Note, 1.95Ref, Note | ||
| Galactic longitude (°) | 18.9779Ref | Proper motion in α (mas/yr) | -0.24±0.03Ref | ||
| Galactic latitude (°) | 0.3828Ref | Proper motion in δ (mas/yr) | -1.93±0.03Ref |
Included in the list of late-type emission-line stars by Allen (1973), these stars were identified as potentially either symbiotic stars or heavily reddened objects. The paper also mentioned that the infrared continuum is dominated by the late-type companion. The star was classified as a Be star in Merrill et al. (1925), a P Cygni-type star in Struve (1944), a B3neq star in Arkhipova (1963), and a B0.5 Ia with emission lines in Vijapurkar & Drilling (1993).