| discov_num |
notes |
refcode |
| BUG 3 |
Liu et al (2008) estimate spectral types T5.0 +/- 0.5 and T5.5 +/- 0.5 |
LiM2008 |
|
and effective temperatures 1028 +/- 17 and 978 +/- 17K. Orbital |
|
|
elements, determined using a Markov Monte Carlo technique, yield |
|
|
masses 0.0287 +/- 0.0016 and 0.0269 +/- 0.0016 Msun. Age of the system |
|
|
is estimated at 0.78 +/- 0.09 Gyr. |
|
|
Assuming a parallactic distance of 13.59 +/- 0.22 pc |
|
|
(Tinney et al. 2003), Konopacky et al. (2010) derive a system mass of |
Bug2003b |
|
0.060 +/- 0.004 Msun. |
Kon2010 |
| refcode |
metd |
author |
reference |
| Bug2003b |
- |
Tinney, C.G., Burgasser, A.J., & Kirkpatrick, J.D. |
2003AJ....126..975T |
| Bug2003b |
|
AJ 126, 975, 2003 |
|
| Kon2010 |
Ag j |
Konopacky, Q.M., Ghez, A.M., Barman, T.S., Rice, E.L., Bailey, III, J.I., |
2010ApJ...711.1087K |
| Kon2010 |
|
White, R.J., McLean, I.S., & Duchene, G. |
|
| Kon2010 |
|
ApJ 711, 1087, 2010 |
|
| LiM2008 |
Ag j |
Liu, M.C., Dupuy, T.J., & Ireland, M.J. |
2008ApJ...689..436L |
| LiM2008 |
+Ha |
ApJ 689, 436, 2008 |
2003ApJ...586..512B |
| LiM2008 |
+Hp |
(included re-reduction of HST data originally published in Bug2003 and Boy2008) |
2008A&A...481..757B |
