discov_num | notes | refcode |
JAO 8 | The fainter source in the STIS UV data is the red dwarf primary; the | |
brighter blue companion is a faint white dwarf with a mass >0.5Msun. | Jao2014a | |
Primary is SCR 1848-6855, a high-proper motion M5.0V dwarf at 24.6pc. | ||
Astrometric observations spanning 8.5 years reveal large photocentric | ||
perturbation due to an initially unseen companion. The pair was | ||
subsequently resolved by HST/STIS. | Jao2014b |
refcode | metd | author | reference |
Jao2014b | C - | Jao, W.-C., Henry, T.J., Subasavage, J.P., Winters, J.G., Gies, D.R., | 2014AJ....147...21J |
Jao2014b | Riedel, A.R., & Ianna, P.A. | ||
Jao2014b | AJ 147, 21, 2014 |
coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
18483-6856 | JAO 8 | 2011 | 1 | 278 | 0.3 | 23.60 | 20.90 | M5.0V+WD | NO P | 184820.97-685535.0 | |
18483-6856 | JAO 8 | 2019 | 2 | 265 | 0.7 | 23.60 | 20.90 | M5.0V+WD | NO P | 184821.10-685532.0 | |
18483-6856 | JAO 8 | 2021 | 3 | 266 | 0.8 | 23.60 | 20.90 | M5.0V+WD | NO P | 184821.10-685532.0 |