January 13, 2024
New objects added
January 17, 2023
Gaia DR3 candidates added
January 15, 2023
Utilities and search added
January 4, 2023
New version fully released
November 7, 2022
New version testing started
Jan 28, 2019
First public release
All symbiotics
Galactic symbiotics
Extragalactic symbiotics
Version from February 3, 2024
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).