WDS 20551-5207 I 18 (HD 198829) : NOTES
 
 
discov_num notes refcode
I 18 The known 3".9 pair I 18 with estimated period ~1700 yr cannot explain
the acceleration. Tok2012a
CPM. Is the acceleration caused by this binary or sub-system? Tok2014d
 
 
REFERENCES
 
 
refcode metd author reference
Tok2012a A j Tokovinin, A., Hartnung, M., Hayward, T.L., & Makarov, V.V. 2012AJ....144....7T
Tok2012a AJ 144, 7, 2012
Tok2014d E2 - Tokovinin, A. 2014AJ....147...86T
Tok2014d AJ 147, 86, 2014
 
 
DISCOVERER
 
 
idgroup discov author
1 I Innes, R.T.A.
5 I MNRAS 57, 533, 1897 (data also in I__1897b,
5 I I__1897c)
 
 
WDS HISTORIC DATA
 
 
coord_2000 discov_num comp epoch obs pa sep mag_pri mag_sec spectr notes coord_arcsec_2000
20551-5207 I 18 1999 8 0 3.6 7.00 10.20 G5 D 205508.17-520710.5
20551-5207 I 18 2011 10 359 4.0 7.00 10.20 G5 D 205508.17-520710.5
20551-5207 I 18 2015 12 359 4.0 7.12 10.20 G5 N 205508.17-520710.5
20551-5207 I 18 2016 14 359 4.0 7.12 10.20 G5 N 205508.17-520710.5

If you need more information about this double, apply for a data request form to the WDS.