discov_num | notes | refcode |
MLB 116 | Triple star with weak hierarchy. Motions of all components relative to | |
each other are small. If we trust the relatively large pm for A from | ||
the WDS, the system is physically bound; however there is an | ||
appreciable discrepancy between this pm and the value given by | ||
Kharhenko & Rezer (2001, Kinemat. Fiz. Nebesn. Tel 17, 409). Therefore | ||
we are not yet able to determine with confidence whether or not the | ||
components are physically bound. | Kiy2012 |
refcode | metd | author | reference |
Kiy2012 | orb - | Kiyaeva, O.V., Kiselev, A.A., Romanenko, L.G., Kalinichenko, O.A. & Vasileva, T.A. | 2012ARep...56..952K |
Kiy2012 | ARep 56, 952, 2012 (SvA 89, 1045, 2012) |
idgroup | discov | author |
1 | MLB | Milburn, W. (Espin, T.E.) |
coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
03279+5625 | MLB 116 | AB | 2001 | 6 | 48 | 3.8 | 10.50 | 10.60 | D | 032755.59+562438.9 | |
03279+5625 | MLB 116 | AB | 2003 | 7 | 47 | 3.8 | 10.50 | 10.60 | D | 032755.59+562438.9 | |
03279+5625 | MLB 116 | AB | 2015 | 18 | 46 | 3.9 | 10.50 | 10.60 | N | 032755.59+562438.9 |