WDS 10425-3340 NHR 1 : NOTES
 
 
discov_num notes refcode
NHR 1 The source at 2.4" separation, first reported in Neuhauser et al. Nhr2000
(2000), is an already known background star (Lowrance et al. 2005), a Lwr2005
conclusion which we can confirm at ~28 sigma confidence. Jnn2012
 
 
REFERENCES
 
 
refcode metd author reference
Jnn2012 Cl j Janson, M., Hormuth, F., Bergfors, C., Brandner, W., Hippler, S., Daemgen, S., 2012ApJ...754...44J
Jnn2012 +E2 Kudryavtseva, N., Schmalzl, E., Schnupp, C., & Henning, T.
Jnn2012 ApJ 754, 44, 2012 (some recalibrated measures published in Jnn2014b) 2014ApJS..214...17J
Lwr2005 H+ j Lowrance, P.J., Becklin, E.E., Schneider, G., Kirkpatrick, J.D., Weinberger, A.J., 2005AJ....130.1845L
Lwr2005 +E2 Zuckerman, B., Dumas, C., Beuzit, J.-L., et al.
Lwr2005 +A AJ 130, 1845, 2005
Lwr2005 +Pp
Nhr2000 Hn j Neuhauser, R., Brandner, W., Eckart, A. Guenther, G., Alves, J., Ott, T., 2000A&A...354L...9N
Nhr2000 +Si Huelamo, N., & Fernandez, M.
Nhr2000 +C A&A 354, L9, 2000
 
 
WDS HISTORIC DATA
 
 
coord_2000 discov_num comp epoch obs pa sep mag_pri mag_sec spectr notes coord_arcsec_2000
10425-3340 NHR 1 1999 3 139 2.5 11.06   M1 104230.06-334016.6
10425-3340 NHR 1 2010 5 119 3.3 11.06   M1 D 104230.06-334016.6
10425-3340 NHR 1 2015 6 114 3.8 7.40 16.80 M1 NU K 104230.06-334016.6

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