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 |
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 |
idgroup | discov | author |
1 | GWP | Garraf Wide Pairs: CPM wide pairs (>50mas/y) discovered in the Garraf Astronomical |
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 |