discov_num | notes | refcode |
JNN 115 | The B component of the system appears to be a close binary itself in | |
several different epochs of AstraLux imaging, but the suspected Ba/Bb | ||
pair is not sufficiently resolved to get a converging binary fit, | ||
hence we treat the AB system as a regular binary in this study. | Jnn2012 |
refcode | metd | author | reference |
Jnn2012 | Cl j | Janson, M., Hormuth, F., Bergfors, C., Brandner, W., Hippler, S., Daemgen, S., | 2012ApJ...754...44J |
Jnn2012 | +E2 | Kudryavtseva, N., Schmalzl, E., Schnupp, C., & Henning, T. | |
Jnn2012 | ApJ 754, 44, 2012 (some recalibrated measures published in Jnn2014b) | 2014ApJS..214...17J |
coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
17380+3330 | JNN 115 | 2009 | 5 | 158 | 1.0 | 11.20 | 12.00 | K7 K7.5 | 173800.75+332946.0 | ||
17380+3330 | JNN 115 | 2015 | 8 | 151 | 1.0 | 11.20 | 12.00 | K7+K7.5 | N | 173800.75+332946.0 |