| discov_num |
notes |
refcode |
| BRG 16 |
The system is precisely at the 3 sigma threshold for statistically |
|
|
significant exclusion of the background star hypothesis. By chance, |
|
|
the AB astrometry is just below the criterion (2.7 sigma) and BC is |
|
|
just above (3.1 sigma), so in principle the BC pair is inconsistent |
|
|
with chance alignment, if the pair does share a common proper motion |
|
|
with A. However, the proper motion of the system has of course been |
|
|
determined based on A, so until the AB physical connection has been |
|
|
demonstrated to the required accuracy, the 3.1 sigma confidence of the |
|
|
BC pair is irrelevant. Hence, we label the entire system as |
|
|
undetermined for now, although it is obviously very likely that the |
|
|
whole system is indeed bound. |
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 |
| idgroup |
discov |
author |
| 1 |
BRG |
Bergfors, C. Brandner, W., Janson, M., Daemgen, S., Geissler, K., Henning, T., |
| 1 |
BRG |
Hippler, S., Hormuth, F., Joergens, V., & Koehler, R. |
| 10 |
BRG |
Bergfors, C. Brandner, W., Daemgen, S., Biller, B., Hippler, S., Janson, M., |
| 10 |
BRG |
Kudryavtseva, N., Geissler, K., Henning, T., & Koehler, R. |
| 11 |
BRG |
Bergfors, C. Brandner, W., Bonnefoy, M., Schlieder, J., Janson, M., Henning, Th. & |
| 11 |
BRG |
Chauvin, G. |
