| discov_num |
notes |
refcode |
| MUG 8 |
Based on astrometry, photometry and H- and K-band spectroscopy, |
|
|
Mugrauer et al. (2007) conclude that HD 65216 A and B comprise a |
Mug2007 |
|
physical pair. The projected separation is 253 au. The Ba and Bb |
|
|
(their B and C) components also appear to be co-moving. From narrow- |
|
|
band photometry of all components, conclude spectral type of Ba is |
|
|
M7-M8 and that of Bb is L2-L3; masses are 0.089 +/- 0.001 and 0.078 |
|
|
+/- 0.001 Msun for Ba and Bb, assuming a system age of 5 Gyr. Orbital |
|
|
period of Ba,Bb estimated at 36y. Theta values estimated from their |
|
|
Figure 6. |
|
|
Primary is planet host star. Two companions Ba and Bb bound to A |
|
|
component. Spectral types of Ba and Bb are M6.5-L0 and M7.5-L4, |
|
|
respectively. |
Egn2007 |
|
AB: A is exoplanet host, P=613d, 5542d |
Tok2014d |
| refcode |
metd |
author |
reference |
| Egn2007 |
Ao j |
Eggenberger, P., Udry, S., Chauvin, G. Beuzit, J.-L., Lagrange, A.-M., Segransan, |
2007A&A...474..273E |
| Egn2007 |
|
D., & Mayor, M. |
|
| Egn2007 |
|
A&A 474, 273, 2007 |
|
| Mug2007 |
Ci j |
Mugrauer, M., Seifahrt, A., & Neuhauser, R. |
2007MNRAS.378.1328M |
| Mug2007 |
+E2 |
MNRAS 378, 1328, 2007 |
|
| Mug2007 |
+A |
|
|
| Tok2014d |
E2 - |
Tokovinin, A. |
2014AJ....147...86T |
| Tok2014d |
|
AJ 147, 86, 2014 |
|
