| discov_num |
notes |
refcode |
| STF1104 |
A premature orbit has been computed for AB. |
|
|
AD: Optical pair, based on study of relative motion of the components |
|
|
using the method of apparent motion parameters. |
Kiy2008 |
| TOK 391 |
Ca,Cb: This is another nearby multiple system. The main component HIP |
|
|
36395 is a visual binary with a known 728yr orbit, also measured here. |
|
|
The C component (NLTT 17952) at 20".4 is physical, and yet another CPM |
|
|
component F is found at 1072" (Tokovinin & Lepine 2012), while the WDS |
Tok2012c |
|
components D and E are optical. We observed C and resolved it at |
|
|
0".09. The orbital period of Ca,Cb is on the order of 6yr, estimated |
|
|
masses are 0.6 and 0.4 Msun. We also targeted F and did not resolve |
|
|
it. The magnitudes and colors of C and F are quite similar. |
Tok2015c |
| STF1104 |
AD: Rectilinear solution by Hurowitz et al. (2013). |
USN2013a |
| refcode |
metd |
author |
reference |
| Kiy2008 |
- |
Kiyaeva, O.V., Kiselev, A.A. & Izmailov, I.S. |
2008SvAL...32..405K |
| Kiy2008 |
|
SvAL 34, 405, 2008 |
|
| Tok2012c |
Pp - |
Tokovinin, A. & Lepine, S. |
2012AJ....144..102T |
| Tok2012c |
+E2 |
AJ 144, 102, 2012 |
|
| Tok2012c |
|
(Note: Per author's suggestion, catalog only includes pairs with Pphys > 0.2 or |
|
| Tok2012c |
|
both proper motions >100 mas/yr. Coarse date of 1980 assumed for all Sky Survey |
|
| Tok2012c |
|
measures. Theta values derived by cataloguer from component coordinates. |
|
| Tok2012c |
|
2MASS photometry replaced with more precise catalog values and errors.) |
|
| Tok2015c |
orb+j |
Tokovinin, A., Mason, B.D., Hartkopf, W.I., Mendez, R.A., & Horch, E.P. |
2015AJ....150...50T |
| Tok2015c |
+St |
AJ 150, 50, 2015 (some measures corrected in Tok2017b) |
2017AJ....154..110T |
| Tok2021c |
orb - |
Tokovinin, A. |
2021IAUDS.203....1S |
| Tok2021c |
|
Inf. Circ. 203, 1, 2021 |
|
| USN2013a |
lin - |
Hurowitz, J.L., Hartkopf, W.I., & Mason, B.D. |
2013IAUDS.181....1H |
| USN2013a |
|
Inf. Circ. 181, 1, 2013 |
|
