| discov_num |
notes |
refcode |
| I 422 |
Light and radial velocity variable. |
|
|
Primary is eclipsing variable V871 Cen (period 2.0842 day). |
Zas2010 |
|
This is another complicated multiple system with three visual pairs at |
|
|
0.36", 1.7", and 9.6". The AB pair further contains an eclipsing |
|
|
binary (Otero 2007, Open European Journal on Variable Stars 72, 1; |
|
|
P=2.08d) and a spectroscopic binary with a period of 2.8d (Sana et al. |
Sna2011a |
|
2011). This brings the number of stars with 10" to six. It is not |
|
|
currently possible to determine which component of the AB pair is the |
|
|
eclipsing one and which is the spectroscopic one. |
Sna2014 |
| refcode |
metd |
author |
reference |
| Sna2011a |
not - |
Sana, H., James, G., & Gosset, E. |
2011MNRAS.416..817S |
| Sna2011a |
|
MNRAS 416, 817, 2011 |
|
| Sna2014 |
Kv j |
Sana, H., LeBouquin, J.-B., Lacour, S., Berger, J.-P., Duvert, G., Gauchet, L., |
2014ApJS..215...15S |
| Sna2014 |
+A |
Norris, B., Olofsson, J., Pickel, D., Zins, G., Absil, O., de Koter, A., |
|
| Sna2014 |
|
Kratter, K., Schnurr, O., & Zinnecker, H. |
|
| Sna2014 |
|
ApJS 215, 15, 2014 |
|
| Sna2014 |
|
(NACO companions in Table 6 assumed physical if quoted probability of spurious |
|
| Sna2014 |
|
detection <10%, optical if >90%, otherwise indeterminate) |
|
| Zas2010 |
- |
Zasche, P. |
................... |
| Zas2010 |
|
private communication, 2010 |
|
