discov_num |
notes |
refcode |
RST1877 |
Carmona et al. (2007) reanalyzed the data obtained by Perez et al. |
Crm2007 |
|
(2004), resulting in a change in his position angle from 353 to 4deg. |
Pez2004 |
|
Muller et al. (2011) resolved the B component into a close pair, which |
MuA2011 |
|
they referred to as BC. However, the C component is a long-known |
|
|
distant member of the system, so the close pair has been renamed |
Glp1892f |
|
MUA 1 Ba,Bb. They derive the following parameters for the close |
|
|
members of the system: |
|
|
component: A Ba Bb |
|
|
spec: F0IIIe K7V M1V |
|
|
L (Lsun) 12.7 +6.4/-3.7 0.50 +0.24/-0.20 0.41 +0.19/-0.16 |
|
|
Teff (K) 7220 +/- 115 4000 +/- 250 3750 +/- 250 |
|
|
M (Msun) 1.8 +0.2/-0.1 0.8 +/- 0.2 0.5 +/- 0.2 |
|
|
R (Rsun) 2.3 +/- 0.5 1.5 +/- 0.7 1.5 +/- 0.7 |
|
|
age (Myr) 9 +/- 2 4 +5/-2 3 +2/-1 |
|
refcode |
metd |
author |
reference |
Crm2007 |
Xr j |
Carmona, A., van den Ancker, M.E., & Henning, T. |
2007A&A...464..687C |
Crm2007 |
+Ci |
A&A 464, 687, 2007 |
|
Glp1892f |
Ma - |
Glasenapp, S. |
1892QB821.G54v1.... |
Glp1892f |
|
Mesures d'Etoiles Doubles, v1, Imp. Acad. Sci. St. Petersburg, 1892 |
|
MuA2011 |
A j |
Muller, A., Carmona, A., van den Ancker, M.E., van Boekel, R., Henning, Th., & |
2011A&A...535L...3M |
MuA2011 |
|
Launhardt, R. |
|
MuA2011 |
|
A&A 535, L3, 2011 |
|
Pez2004 |
C - |
Perez, M.R., van den Ancker, M.E., de Winter, D., & Bopp, B.W. |
2004A&A...416..647P |
Pez2004 |
+Ci |
A&A 416, 647, 2004 |
|