discov_num |
notes |
refcode |
RAO 22 |
Acceleration binary (Makarov & Kaplan 2005) first resolved by Riddle |
Mkr2005 |
|
et al. (2015). The position angle in this paper measured on 2013.8367 |
RAO2015 |
|
differs by 27° from the 2012.7592 measurement. That is not the only |
|
|
discrepancy between the two data sets. The photometry with P3K shows |
|
|
large magnitude differences (dJ = 2.5 and dK = 2.3), while Robo-AO |
|
|
detected a binary of equal brightness. The separation between the two |
|
|
components is fairly small and in the P3K data, the companion lies on |
|
|
the Airy ring of the primary, which could increase the errors. The |
|
|
primary is a high PM star, the pair AB is most likely a physical |
|
|
binary. Additional observations are needed to understand this system. |
Rbr2015d |
refcode |
metd |
author |
reference |
Mkr2005 |
- |
Makarov, V.V. & Kaplan, G.H. |
2005AJ....129.2420M |
Mkr2005 |
|
AJ 129, 2420, 2005 |
|
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 |
|