| discov_num |
notes |
refcode |
| DAE 3 |
RBS 887 |
|
|
Daemgen et al. (2007) derive distance of 19.6 +/- 4.6 pc, separations |
|
|
of 20.8 +/- 6.0 au (AB) and 3.7 +/- 1.1 au (BC), and predicted orbital |
|
|
periods of 157 +97/-93 yr (AB) and 16 +10/-9 yr (BC). Spectral types |
|
|
for the three components are M3.5 +/- 0.5, M4.5 +/- 0.5, and M4.5 +/- |
|
|
0.5; masses 0.29 +0.11/-0.08, 0.16 +0.05/-0.04, 0.16 +0.05/-0.0 Msun. |
Dae2007 |
|
2MASS J10364483+1521394 is a triple in the Ursa Major moving group, |
|
|
consisting of a low-mass M dwarf orbited by 2 less-massive companions. |
|
|
Calissendorff et al. (2017) derive orbits for the BC pair, as well as |
|
|
A,BC. The semimajor axis for BC is 161 +/- 2 AU; combined mass for the |
|
|
pair is 0.482 +/- 0.145 Msun. If the BC dynamical mass is constrained |
|
|
to this value, an orbital solution for A,BC yields a semimajor axis of |
|
|
38 +/- 4A U and a system mass of 1.00 +/- 0.03 Msun for the triple. |
|
|
The mass of A is 0.53 +/- 0.20 Msun, while B and C have similar masses |
|
|
of 0.24 +/- 0.07 Msun each. |
Jnn2017b |
| refcode |
metd |
author |
reference |
| Dae2007 |
A j |
Daemgen, S., Siegler, N., Reid, I.N., & Close, L.M. |
2007ApJ...654..558D |
| Dae2007 |
|
ApJ 654, 558, 2007 |
|
| Jnn2017b |
Cl j |
Calissendorff, P., Janson, M., Kohler, R., Durkan, S., Hippler, S., Dai, X., |
2017A&A...604A..82C |
| Jnn2017b |
+orb |
Brandner, W., Schlieder, J., & Henning, T. |
|
| Jnn2017b |
|
A&A 604, A82, 2017 |
|
