discov_num | notes | refcode |
JNN 53 | The companion that was detected in the AstraLux images has not yet | |
been confirmed as a physical companion through common proper motion. | ||
However, the two components have nearly equal brightness and colors, | ||
and a relatively small separation of ~1.4" hence it is very likely | ||
that it is a real physical binary, and it is counted as such here for | ||
statistical purposes. | 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 |
06283-0111 | JNN 53 | 2009 | 3 | 153 | 1.4 | 13.40 | 13.40 | M2 M2 | 062818.61-011050.3 | ||
06283-0111 | JNN 53 | 2016 | 4 | 153 | 1.4 | 13.40 | 13.40 | M2+M2 | NV | 062818.61-011050.3 |