discov_num | notes | refcode |
SCE 1 | GJ 660.1 = GJ 9588. Schneider et al. (2011) estimate spectral type of | |
the secondary as M9 +/- 2. Projected separation is 120 +/- 9 au. | Sce2011 | |
Aganze et al (2016) derive spectral types M1 and d/sdM7 and effective | ||
temperatures 3800 and 2550 +80/-90 K. Masses are 0.57 +/- 0.07 and | ||
0.084-0.091 Msun, radii 0.53 +/- 0.04 and 0.085 +/- 0.014 Rsun. The | ||
authors suggest the possibility that unusual spectral features of the | ||
B component may arise from contamination due to an additional | ||
unresolved companion. | Bug2016 |
refcode | metd | author | reference |
Bug2016 | not - | Aganze, Ch., Burgasser, A.J., Faherty, J.K., Choban, C., Escala, I., Lopez, M.A., | 2016AJ....151...46A |
Bug2016 | Jin, Y., Tamiya, T., Tallis, M., & Rockward, W. | ||
Bug2016 | AJ 151, 46, 2016 | ||
Sce2011 | Ci j | Schneider, A., Melis, C., Song, I., & Zuckerman, B. | 2011ApJ...743..109S |
Sce2011 | ApJ 743, 109, 2011 |
coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
17129-0508 | SCE 1 | 2009 | 3 | 353 | 6.1 | 8.66 | 13.20 | M1V+d/sdM | N | 171251.26-050731.3 | |
17129-0508 | SCE 1 | 2015 | 4 | 351 | 5.9 | 8.66 | 13.20 | M1V+d/sdM | N | 171251.26-050731.3 | |
17129-0508 | SCE 1 | 2016 | 5 | 351 | 5.9 | 8.66 | 13.20 | M1V+d/sdM | N | 171251.26-050731.3 |