| discov_num |
notes |
refcode |
| STF1932 |
There is evidence of light-variability in the system. |
|
|
A subsystem of 30 to 50 yr period, formerly suspected from visual |
|
|
data, is not supported by the more recent observations. |
|
|
See Baize & Petit (1989) catalog of doubles with variable component. |
Baz1989d |
|
Spectral types and masses of components assigned by ten Brummelaar et |
TtB2000 |
|
al., based on adaptive optics observations. |
|
|
AB: Check astrometric orbit of Ba,Bb. Interferometric observations do |
|
|
not support 30-y or 50-y astrometric subsystem. |
Tok2014d |
| refcode |
metd |
author |
reference |
| Baz1989d |
- |
Baize, P. & Petit, M. |
1989A&AS...77..497B |
| Baz1989d |
|
A&AS 77, 497, 1989 |
|
| Tok2014d |
E2 - |
Tokovinin, A. |
2014AJ....147...86T |
| Tok2014d |
|
AJ 147, 86, 2014 |
|
| TtB2000 |
Ac j |
ten Brummelaar, T.A., Mason, B.D., McAlister, H.A., Roberts, L.C., Jr., |
2000AJ....119.2403T |
| TtB2000 |
|
Turner, N.H., Hartkopf, W.I., & Bagnuolo, W.G., Jr. |
|
| TtB2000 |
|
AJ 119, 2403, 2000 (magnitude differences from Mt. Wilson AO) |
|
