| discov_num |
notes |
refcode |
| STF1102 |
AB: HJL 84. |
HJL1986 |
|
AD: HJL1048. |
HJL1986 |
|
AD: SHY 191. Bayesian analysis by Shaya & Olling (2011) indicates very |
Shy2011 |
|
high (near 100%) probability pair is physical. |
|
|
AD: Halbwachs et al. (2012): SB1 orbit of D, P=2708.2d, e=0.716, |
HJL2012b |
|
K1=4.93, V0=-2.38 => M2min=0.27. D co-moving with HIP 33818 at 6.0pc. |
Tok2014d |
|
BD: HJL1049. |
HJL1986 |
| TOK 392 |
Da,Db: This is a quadruple system. The 7".7 AB pair (STF 1102) is |
|
|
HIP 36485, the CPM component D = HIP 36497 = HD 59450 is located at |
|
|
112" from it, while the WDS components C and E are optical. The |
|
|
physical nature of AD is established by common PM, distance, and RV. |
|
|
D is a known SB1 with P=2708d=7.4yr (Halbwachs et al. 2012, MNRAS 422, |
|
|
14) and an estimated semi-major axis of 93mas, also an acceleration |
|
|
binary. We resolved the Da,Db pair at 0".11, dI=2.6. The minimum mass |
|
|
of Db derived from its SB orbit is 0.27 Msun, while we estimate the |
|
|
masses of Da and Db as 1.05 and 0.6 Msun from their luminosity. A |
|
|
previous non-resolution of D is reported in INT4; it was also |
RAO2015 |
|
unresolved with Robo-AO (Riddle et al. 2015). |
Tok2015c |
| refcode |
metd |
author |
reference |
| HJL1986 |
Pa - |
Halbwachs, J.L. |
1986A&AS...66..131H |
| HJL1986 |
|
A&AS 66, 131, 1986 |
|
| HJL1986 |
|
(Possible CPM pairs from AGK2/3. Coarse astrometry, incl. mean 1950 dates, added |
|
| HJL1986 |
|
only for previously unknown pairs. Table 1: HJL 1 - 326, Table 2: HJL1001 - 1113) |
|
| HJL2012b |
not - |
Halbwachs, J.L., Mayor, M., & Udry, S. |
2012MNRAS.422...14H |
| HJL2012b |
|
MNRAS 422, 14, 2012 |
|
| 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.) |
|
| Shy2011 |
- |
Shaya, E.J. & Olling, R. |
2011ApJS..192....2S |
| Shy2011 |
|
ApJS 192, 2, 2011 |
|
| Shy2011 |
|
(Statistical analysis of probability that wide Hipparcos pairs are physical. Pairs |
|
| Shy2011 |
|
added to WDS only if probability 90% or greater.) |
|
| Tok2014d |
E2 - |
Tokovinin, A. |
2014AJ....147...86T |
| Tok2014d |
|
AJ 147, 86, 2014 |
|
| 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 |
