| discov_num |
notes |
refcode |
| RAO 40 |
Primary is SB, P=49.480d. Estim. mass of B 0.26 Msun. |
Tok2014d |
|
Triple system with inner 74.1 day spectroscopic pair (Gorynya & |
|
|
Tokovinin 2014 MNRAS 441, 2316) and tertiary from Riddle et al. (2015) |
RAO2015 |
|
confirmed as physical by our photometry and astrometry. Observations |
|
|
demonstrate that photometry of B given in 2MASS is biased by proximity |
|
|
of bright primary, as in many other similar pairs. Their "unusual" |
|
|
colors derived from the 2MASS photometry are thus wrong. |
Rbr2015d |
| refcode |
metd |
author |
reference |
| RAO2015 |
Ag u |
Riddle, R.L., Tokovinin, A., Mason, B.D., Hartkopf, W.I., Roberts, L.C., Jr., |
2015ApJ...799....4R |
| RAO2015 |
+orb |
Baranec, C., Law, N.M., Bui, K., Burse, M.P., Das, H.K., Dekany, R.G., |
|
| RAO2015 |
|
Kulkarni, S., Punnadi, S., Ramaprakash, A.N., & Tendulkar, S.P. |
|
| RAO2015 |
|
ApJ 799, 4, 2015 |
|
| RAO2015 |
|
(Note: Paper includes separation/magnitude difference limits for all stars |
|
| RAO2015 |
|
observed. These limits have been added to the Interferometric Catalog even for |
|
| RAO2015 |
|
resolved pairs, to indicate restrictions on any potential additional components.) |
|
| Rbr2015d |
Ac j |
Roberts, L.C., Jr., Tokovinin, A., Mason, B.D., Hartkopf, W.I., & Riddle, R.L. |
2015AJ....150..130R |
| Rbr2015d |
+A |
AJ 150, 130, 2015 |
|
| Tok2014d |
E2 - |
Tokovinin, A. |
2014AJ....147...86T |
| Tok2014d |
|
AJ 147, 86, 2014 |
|
