| discov_num |
notes |
refcode |
| STF2474 |
B is BD+34 3438. |
|
|
AB: NLTT 47474/47473 |
Chm2004 |
|
AB: B is exoplanet host, P=71.5d. |
Tok2014d |
| CHR 84 |
Aa,Ab: 1985.5232: This autocorrelogram was remeasured; the new results |
|
|
are listed here. |
|
|
The paper by Tokovinin et al. (2000) also includes a combined |
Tok2000a |
|
spectroscopic/astrometric solution for orbital elements and masses. |
|
|
Aa,Ab: Malkov et al. (2012) derive dynamical, photometric, and |
|
|
spectroscopic masses 5.43 +/- 2.10, 2.39, and 1.02 Msun, respectively. |
Mlk2012 |
|
Aa,Ab: SB2, P=3.540y. |
Tok2014d |
|
Combined solution by Farrington et al. (2014) yields masses 0.802 +/- |
|
|
0.055 and 0.622 +/- 0.053 Msun, as well as an orbital parallax 28.26 |
|
|
+/- 1.70 mas. |
CIA2014a |
| refcode |
metd |
author |
reference |
| Chm2004 |
E - |
Chaname, J. & Gould, A. |
2004ApJ...601..289C |
| Chm2004 |
|
ApJ 601, 289, 2004 |
|
| Chm2004 |
|
(Photometry, coordinates, and astrometry from rNLTT. Astrometry from early |
|
| Chm2004 |
|
versions of 2MASS and UCAC, with date given only as "circa 2000". Measures |
|
| Chm2004 |
|
identical to discovery observations - predominantly close pairs - were assumed |
|
| Chm2004 |
|
not new observations, so not included in WDS. Similar concerns when primary and |
|
| Chm2004 |
|
secondary magnitudes or proper motions were the same.) |
|
| CIA2014a |
Kf j |
Farrington, C.D., ten Brummelaar, T.A., Mason, B.D., Hartkopf, W.I., Mourard, D., |
2014AJ....148...48F |
| CIA2014a |
+Kc |
Moravveji, E., McAlister, H.A., Turner, N.H., Sturmann, L., & Sturmann, J. |
|
| CIA2014a |
+orb |
AJ 148, 48, 2014 |
|
| Mlk2012 |
not - |
Malkov, O.Yu., Tamazian, V.S., Docobo, J.A., & Chulkov, D.A. |
2012A&A...546A..69M |
| Mlk2012 |
|
A&A 546, A69, 2012 |
|
| Tok2000a |
S u |
Tokovinin, A.A., Griffin, R.F., Balega, Y.Y., Pluzhnik, E.A., & Udry, S. |
2000AstL...26..116T |
| Tok2000a |
+orb |
SvAL 26, 116, 2000 |
|
| Tok2014d |
E2 - |
Tokovinin, A. |
2014AJ....147...86T |
| Tok2014d |
|
AJ 147, 86, 2014 |
|
