MISCLASSIFIED
MILKY WAY
|
| BD+14 3887 | IRAS 19192+1447 | GSC2.4.2 N2CE000038 | AAVSO 000-BDF-754 |
| SIMBAD BD+14 3887 | Pan-STARRS 125852903916039539 | SAO - | VSX 2568 |
| GAIA DR3 4319930096909297664 | SkyMapper - | WRAY - | GCVS V1429 Aql |
| 2MASS J19213397+1452570 | HIP - | Hen 3-1745 | BD +14 3887 |
| WISE J192133.97+145257.1 | TYC 1054-441-1 | 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 (°) | 290.3916Ref | Parallax (mas) | 0.222±0.020Ref | Reddening E(B-V) (mag) | 4.63±0.14Ref, Note |
| Declination (°) | 14.8825Ref | Distance (kpc) | 3.84Ref, Note, 3.80Ref, Note | ||
| Galactic longitude (°) | 49.5715Ref | Proper motion in α (mas/yr) | -2.14±0.02Ref | ||
| Galactic latitude (°) | 0.2502Ref | Proper motion in δ (mas/yr) | -4.97±0.02Ref |
Included in the list of late-type emission-line stars in Allen (1973), these stars may be either symbiotic stars or heavily reddened objects, according the author. Previously identified as a peculiar Be star in Swensson (1943) and a Bep star in Henize (1976). Additionally, it has been classified as a high-luminosity Be star in Miroshnichenko (1996).