| discov_num |
notes |
refcode |
| BNK 11 |
EQ Cha. Koehler & Petr-Gotzens (2002) suspected duplicity but were |
Koh2002 |
|
unable to split the pair. |
|
|
More commonly known as EQ Cha, this star appears single in the |
|
|
AstraLux images, but has most likely been partially resolved as close |
|
|
binary in previous imaging campaigns (Kohler & Petr-Gotzens 2002; |
Koh2002 |
|
Brandeker et al. 2006). With an angular separation as small as 40 mas |
Bnk2006 |
|
in 2003, it is fully plausible that the companion exists but was too |
|
|
close to be resolved by AstraLux in 2010. |
Jnn2012 |
| refcode |
metd |
author |
reference |
| Bnk2006 |
A j |
Brandeker, A., Jayawardhana, R., Khavari, P., Haisch, K.E., & Mardones, D. |
2006ApJ...652.1572B |
| Bnk2006 |
+E2 |
ApJ 652, 1572, 2006 |
|
| 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 |
| Koh2002 |
Ci j |
Koehler, R. & Petr-Gotzens, M.G. |
2002AJ....124.2899K |
| Koh2002 |
+Si |
AJ 124, 2899, 2002 |
|
| Koh2002 |
+A |
|
|
