WDS 00197+1951 GWP 40 : NOTES
 
 
discov_num notes refcode
GWP 40 XMI 120. Tob2012b
2MASS J00193931+1951050 and J00194303+1951117 are separated by only
53", have very similar proper motions (e.g. Roser et al. 2010) and XXX2010
have similar estimated spectroscopic distances (23 and 21 pc,
respectively) in Riaz et al. (2006), hence it is highly likely that Ria2006
they form a physical pair. 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
Ria2006 not - Riaz, B., Gizis, J., & Harvin, J. 2006AJ....132..866R
Ria2006 AJ 132, 866, 2006
Tob2012b not - Tobal, T. ...................
Tob2012b private communication, 2012
XXX2010 not - Roser, S., Demleitner, M., & Schilbach, E. 2010AJ....139.2440R
XXX2010 AJ, 139, 2440, 2010
 
 
DISCOVERER
 
 
idgroup discov author
1 GWP Garraf Wide Pairs: CPM wide pairs (>50mas/y) discovered in the Garraf Astronomical
 
 
WDS HISTORIC DATA
 
 
coord_2000 discov_num comp epoch obs pa sep mag_pri mag_sec spectr notes coord_arcsec_2000
00197+1951 GWP 40 1998 2 263 53.0 14.90 15.00 N D 001943.03+195112.0
00197+1951 GWP 40 2000 3 263 52.9 14.90 15.00 N D 001943.03+195112.0
00197+1951 GWP 40 2009 4 263 52.9 14.90 15.00 M5+M5 N 001943.03+195112.0
00197+1951 GWP 40 2015 6 263 52.8 14.90 15.00 M5+M5 NV 001943.03+195112.0
00197+1951 GWP 40 2016 8 263 53.1 14.90 15.00 M5+M5 NV 001943.03+195112.0

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