| discov_num |
notes |
refcode |
| CRZ 2 |
BDK 2. G 171-58 + 2MASS J00250365+4759191. Distance 42.2 +2.0/-1.8 |
|
|
pc for primary, 31 +/- 6 pc for secondary. Estimated ages of |
|
|
components are discrepant: 1.8-3.5 Gyr for primary, versus 0.1-0.5 Gyr |
|
|
for secondary. The primary is a spectroscopic binary resolved by |
Hip1997a |
|
Hipparcos, the secondary a close (~10au) L4+L4 pair, resolved by Reid |
Red2006b |
|
(2006). |
Fah2010 |
| HDS 56 |
Aa,Ab: Malkov et al. (2012) derive dynamical, photometric, and |
|
|
spectroscopic masses 1.30 +/- 0.21, 1.85, and 1.10 Msun, respectively. |
Mlk2012 |
| RED 14 |
Ba,Bb: 2MASS J00250365+4759191. Spectral types L4 and L4 |
Red2006b |
| refcode |
metd |
author |
reference |
| Fah2010 |
C - |
Faherty, J.K., Burgasser, A.J., West, A.A., Bochanski, J.J., Cruz, K.L., Shara, . |
2010AJ....139..176F |
| Fah2010 |
|
M.M., & Walter, F.W |
|
| Fah2010 |
|
AJ 139, 176, 2010 |
|
| HIP1997a |
Hh - |
Hipparcos |
1997yCat.1239....0E |
| HIP1997a |
|
Hipparcos Catalog, ESA SP-1200, 1997 (incl. Hp photometry, vol. 10) |
|
| Mit2024 |
S - |
Mitrofanova, A., Dyachenko, V., Beskakotov, A., Balega, Y., Maksimov, A. & |
2024RAA....24i5013M |
| Mit2024 |
+orb |
|
|
| Mit2024 |
|
Research in Astronomy and Astrophysics 24, id.095013, 2024 |
|
| Mlk2012 |
not - |
Malkov, O.Yu., Tamazian, V.S., Docobo, J.A., & Chulkov, D.A. |
2012A&A...546A..69M |
| Mlk2012 |
|
A&A 546, A69, 2012 |
|
| Red2006b |
Hn j |
Reid, I.N., Lewitus, E., Allen, P., Cruz, K.L., & Burgasser, A.J., |
2006AJ....132..891R |
| Red2006b |
+E2 |
AJ 132, 891, 2006 |
|
| discov |
author |
| CRZ |
Cruz, K.L., Reid, I.N., Kirkpatrick, J.D., Burgasser, A.J. Liebert, J., |
| CRZ |
Solomon, A.R., Schmidt, S.J., Allen, P.R., Hawley, S.L., & Covey, K.R. |
| FAH |
Faherty, J.K., Goodman, S., Caselden, D., Colin, G., Kuchner, M.J., Meisner, A.M., |
| FAH |
Gagne, J., Schneider, A.C., Gonzales, E.C., Bardalez Gagliuffi, D.C., Logsdon, S.E., |
| FAH |
ApJ 889, 176, 2020 |
| HIP |
(non-component double star solution: G = acceleration solution, |
| HIP |
O = orbit solution, V = variability-induced mover, X = stochastic solution) |
| MIT |
Mitrofanova, A., Dyachenko, V., Beskakotov, A., Balega, Y., Maksimov, A., |
| MIT |
AJ 159, 266, 2020 |
| RED |
Reid, I.N., Lewitus, E., Allen, P., Cruz, K.L., & Burgasser, A.J., |
| RED |
AJ 132, 891, 2006 |
