discov_num |
notes |
refcode |
PIN 10 |
Secondary is M9V, pm -0.30 +/- 0.02, 0.21 +/- 0.01 arcsec/yr, distance |
|
|
34 +/- 2pc. Given the van Leeuwen (2007) proper motion (-0.296 +/- |
VlF2007 |
|
0.001, 0.203 +/- 0.002 arcsec/yr) and distance (31 +/- 1pc) for the |
|
|
primary, the pair is likely a true CPM system. At a projected |
|
|
separation of 3800 au, the gravitational binding energy makes this one |
|
|
of the most fragile binaries known. |
Thn2013 |
refcode |
metd |
author |
reference |
Thn2013 |
Hw - |
Thompson, M.A., Kirkpatrick, J.D., Mace, G.N., Cushing, M.C., Gelino, C.R., |
2013PASP..125..809T |
Thn2013 |
|
Griffith, F.L., Skrutskie, M.F., Eisenhardt, P.R.M., Wright, E.L., Marsh, K.A., |
|
Thn2013 |
|
Mix, K.J., Beichman, C.A., et al. |
|
Thn2013 |
|
PASP 125, 809, 2013 (no new data) |
|
VlF2007 |
- |
van Leeuwen, F. |
2007A&A...474..653V |
VlF2007 |
|
A&A 474, 653, 2007 |
|
idgroup |
discov |
author |
1 |
PIN |
Pinfield, D.J., Jones, H.R.A., Lucas, P.W., Kendall, T.R., Folkes, S.L., |
1 |
PIN |
Day-Jones, A.C., Chappelle, R.J., & Steele, I.A. |
2 |
PIN |
Pinfield, D.J., Burningham, B., Lodieu, N., Leggett, S.K., Tinney, C.G., |
2 |
PIN |
van Spaandonk, L., Marocco, F., Smart, R., Gomes, J., Smith, L., Lucas, P.W., |
2 |
PIN |
Day-Jones, A.C., et al. |