MISCLASSIFIED
MILKY WAY
|
del Sge | IRAS 19451+1824 | GSC2.4.2 N1TZ000111 | AAVSO 000-BCH-941 |
SIMBAD * del Sge | Pan-STARRS - | SAO 105259 | VSX 27700 |
GAIA DR3 1824534959611831680 | SkyMapper - | WRAY - | GCVS del Sge |
2MASS J19472326+1832034 | HIP 97365 | Hen - | BD +18 4240B |
WISE J194723.26+183203.4 | TYC 1619-3542-1 | ESO - | HD 187077 |
Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
Right ascension (°) | 296.8470Ref | Parallax (mas) | 5.967±0.260Ref | Reddening E(B-V) (mag) | 0.61±0.03Ref, Note |
Declination (°) | 18.5343Ref | Distance (kpc) | 0.17Ref, Note, 0.17Ref, Note | ||
Galactic longitude (°) | 55.7669Ref | Proper motion in α (mas/yr) | 7.28±0.24Ref | ||
Galactic latitude (°) | -3.3834Ref | Proper motion in δ (mas/yr) | 0.32±0.23Ref |
This binary system is suggested to be composed of an M2 II giant and an A0 V star with an orbital period of 3725 days, as reported in Sahade (1986). Pugh et al. (2015) determined a period of 3703.7 days. It is also classified as a VV Cephei-like system, according to Pantaleoni González et al. (2020).