MISCLASSIFIED
MILKY WAY
|
| Hen 2-325 | IRAS - | GSC2.4.2 S9S6005471 | AAVSO - |
| SIMBAD Hen 2-325 | Pan-STARRS 76372702762071634 | SAO - | VSX - |
| GAIA DR3 4064005326584261376 | SkyMapper - | WRAY - | GCVS - |
| 2MASS J18010628-2621257 | HIP - | Hen 2-325 | BD - |
| WISE J180106.27-262125.4 | TYC - | ESO 521-9 | HD - |
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | VDS 111 (Susp.) |
| Right ascension (°) | 270.2763Ref | Parallax (mas) | 0.624±0.019Ref | Reddening E(B-V) (mag) | 3.52±0.17Ref, Note |
| Declination (°) | -26.3573Ref | Distance (kpc) | 1.59Ref, Note, 1.58Ref, Note | ||
| Galactic longitude (°) | 3.9629Ref | Proper motion in α (mas/yr) | 0.30±0.02Ref | ||
| Galactic latitude (°) | -1.6450Ref | Proper motion in δ (mas/yr) | -3.28±0.02Ref |
Listed among possible symbiotic stars in Vaidis (1988), likely due to the reported spectral type Mep + B by Sanduleak & Stephenson (1973) and its inclusion in the catalog of Allen & Glass (1974). Although initially considered a possible PN in Henize (1967), this classification was refuted by Acker et al. (1987) and Stenholm & Acker (1987). The object was subsequently reclassified as an M-type emission line star in Kohoutek (2001). A spectrum presented in Pereira et al. (2003) displayed several hydrogen and helium absorption lines, leading to its categorization as a reddened Be star.