MISCLASSIFIED
MILKY WAY
|
V1710 Aql | IRAS 18594+0204 | GSC2.4.2 N1O6000132 | AAVSO 000-BKD-028 |
SIMBAD SH 2-71 | Pan-STARRS 110582855012594147 | SAO - | VSX 63096 |
GAIA DR3 4268419106711771776 | SkyMapper - | WRAY - | GCVS V1710 Aql |
2MASS J19020029+0209109 | HIP - | Hen - | BD - |
WISE J190200.28+020910.9 | TYC - | ESO - | HD - |
Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | Sh 2-71 (Susp.) |
Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
Right ascension (°) | 285.5012Ref | Parallax (mas) | 0.625±0.018Ref | Reddening E(B-V) (mag) | 3.82±0.2Ref, Note |
Declination (°) | 2.1530Ref | Distance (kpc) | 1.50Ref, Note, 1.50Ref, Note | ||
Galactic longitude (°) | 36.0534Ref | Proper motion in α (mas/yr) | -0.78±0.02Ref | ||
Galactic latitude (°) | -1.3672Ref | Proper motion in δ (mas/yr) | -3.49±0.02Ref |
Included as a suspected symbiotic star in the catalog of Akras et al. (2019) with a reference to the paper by Corradi et al. (2011); however, it should be noted that the mentioned paper pertains to M 2-9, which is a different object. In Mikulášek et al. (2007), it was claimed that the object has a very dense inner nebula, similar to that seen in symbiotic binaries. However, V1710 Aql is more likely a planetary nebula with a triple central star, as suggested in Jones et al. (2019).