WDS 10232+0542 TOK 200 Aa,Ab : NOTES
discov_num |
notes |
refcode |
SHJ 115 |
Optical pair, based on study of relative motion of the components |
|
|
using the method of apparent motion parameters. |
Kiy2008 |
|
H 5 64. |
MEv2010 |
TOK 200 |
The 1".1 speckle companion can explain dmu, but not the acceleration. |
Tok2012a |
REFERENCES
refcode |
metd |
author |
reference |
Kiy2008 |
- |
Kiyaeva, O.V., Kiselev, A.A. & Izmailov, I.S. |
2008SvAL...32..405K |
Kiy2008 |
|
SvAL 34, 405, 2008 |
|
MEv2010 |
- |
MacEvoy, B. |
................... |
MEv2010 |
|
private communication, 2010 (see http://www.handprint.com/ASTRO/index.html) |
|
Tok2012a |
A j |
Tokovinin, A., Hartnung, M., Hayward, T.L., & Makarov, V.V. |
2012AJ....144....7T |
Tok2012a |
|
AJ 144, 7, 2012 |
|
DISCOVERER
idgroup |
discov |
author |
1 |
SHJ |
South, J. & Herschel, J. |
WDS HISTORIC DATA
coord_2000 |
discov_num |
comp |
epoch |
obs |
pa |
sep |
mag_pri |
mag_sec |
spectr |
notes |
coord_arcsec_2000 |
10232+0542 |
TOK 200 |
Aa,Ab |
2011 |
1 |
333 |
1.1 |
6.57 |
12.00 |
F6V |
N |
102314.61+054139.2 |
10232+0542 |
TOK 200 |
Aa,Ab |
2014 |
2 |
334 |
1.1 |
6.57 |
12.00 |
F6V |
N |
102314.61+054139.2 |
10232+0542 |
TOK 200 |
Aa,Ab |
2019 |
3 |
336 |
1.0 |
6.57 |
12.00 |
F6V |
N |
102314.61+054139.2 |
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