| discov_num |
notes |
refcode |
| JNN 24 |
This is a close triple system discovered with AstraLux, where in |
|
|
particular the tertiary component is difficult to fit for. Since the |
|
|
relative positions of the BC pair components are therefore clearly |
|
|
dominated by noise scatter in both separation and position angle, we |
|
|
set the error of each epoch to the scatter among the data points and |
|
|
make no assessment of orbital motion for the BC pair (although by |
|
|
contrast, clear orbital motion is seen of the pair with respect to the |
|
|
A component). |
Jnn2012 |
|
Estimated age 10-20 Myr; masses 0.07 +/- 0.01 and 0.04 +/- 0.01 Msun; |
|
|
a ~8.7 au. |
Jnn2014 |
| 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 |
| Jnn2014 |
A - |
Janson, M., Bergfors, C., Brandner, W., Kudryavtseva, N., Hormuth, F., |
2014ApJ...789..102J |
| Jnn2014 |
+Cl |
Hippler, S., & Henning, T. |
|
| Jnn2014 |
|
ApJ 789, 102, 2014 |
|
