WDS 06562+4032 RAO 56 AC : NOTES
 
 
discov_num notes refcode
RBR 28 Primary has a slow PM of 0".037/y. The Riddle et al. (2015) companion RAO2015
at 5".6 is located below the MS and could be optical, despite moderate
crowding. We discovered another similarly faint star at 1".9 which was
not spotted in the Robo-AO i'-band image. Little can be said about its
status. The main target itself is a close spectroscopic binary (D.
Latham 2012, private communication) and an X-ray source. Rbr2015d
 
 
REFERENCES
 
 
refcode metd author reference
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.)
Rbr2015d Ac j Roberts, L.C., Jr., Tokovinin, A., Mason, B.D., Hartkopf, W.I., & Riddle, R.L. 2015AJ....150..130R
Rbr2015d +A AJ 150, 130, 2015
 
 
WDS HISTORIC DATA
 
 
coord_2000 discov_num comp epoch obs pa sep mag_pri mag_sec spectr notes coord_arcsec_2000
06562+4032 RAO 56 AC 2013 2 158 5.6 7.62 14.00 F7VgF6mF5 065614.74+403212.8
06562+4032 RAO 56 AC 2015 3 158 5.6 7.62 14.00 F7VgF6mF5 N 065614.74+403212.8

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