| discov_num |
notes |
refcode |
| YLW 11 |
AB: IR sources in rho Oph cloud. WL 20. |
|
|
WL 20E, WL 20W, and WL 20S are the A, B, and C components, |
|
| RES 1 |
respectively. Astrometry based on average of data taken through three |
|
| RIE 1 |
BC: filters: 7900+/-760, 10300+/-1010, 12500+/-1160nm. See Ressler et |
Res2001 |
|
al. (2001) for fluxes of all components at various wavelengths, as |
|
|
well as extensive discussion of system. Duplicity of WL 20 was |
|
|
discovered by Rieke et al (1989), although no astrometric measurements |
Rie1989 |
|
are listed in their paper. |
|
