| discov_num |
notes |
refcode |
| BRG 4 |
The primary star in the system is a known eclipsing binary with a |
|
|
period of 0.4455 days (Parihar et al. 2009 MNRAS 395, 593). Since the |
|
|
angular separation is inside of our inner cut-off, we count the system |
|
|
as a binary here for the purpose of multiplicity statistics, although |
|
|
it is really a triple system. To estimate the mass of the primary for |
|
|
the purpose of deriving the mass ratio to the tertiary component |
|
|
detected in our images, we use the sum of the masses corresponding to |
|
|
individual spectral types M1 and M3 derived for the eclipsing binary. |
Jnn2012 |
|
ASAS J011328-3821.1, eclipsing binary of Algol-type, period 0.44559d. |
Zas2016 |
| 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 |
| Zas2016 |
not - |
Zasche, P. |
................... |
| Zas2016 |
|
private communication, 2016 |
|
| 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. |
