| discov_num |
notes |
refcode |
| TOK 301 |
HIP 76400 is identified by the GCS as an SB2 with a mass ratio q=0.93, |
|
|
but there is no spectroscopic orbit available. We resolved the 0".19 |
|
|
pair with dI=3.9, indicating a mass ratio of ~0.5 and an orbital |
|
|
period of ~30yr. Very likely the resolved binary does not match the |
|
|
spectroscopic double-lined system. Considering the CPM component B at |
|
|
80" (Tokovinin & Lepine 2012), this system could be a quadruple with a |
Tok2012c |
|
3-tier "3+1" hierarchy. |
Tok2015c |
|
Aa1,Aa2 has a period of 368d. |
Tok2022e |
| refcode |
metd |
author |
reference |
| 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 |
| Tok2021f |
orb - |
Tokovinin, A. |
2021IAUDS.204....1T |
| Tok2021f |
|
Inf. Circ. 204, 1, 2021 |
|
| Tok2022e |
orb |
Tokovinin, A. |
2022AJ....163..161T |
| Tok2022e |
|
AJ 163, 161, 2022 |
|
