| discov_num |
notes |
refcode |
| A 1377 |
Mt. Wilson spectral classes A is G5, C is B8n. |
|
|
AB. This appears to be part of a triple system. The elements given by |
|
|
Wilson (1950) and by Baize (1958) are different, possibly due to the |
WRH1950b |
|
long period of the system. This 1975.533 separation is less than that |
Baz1958 |
|
derived from either ephemeris but it and the position angle are closer |
|
|
to Baize's values. |
BLM1978 |
|
2003.6: Differential astrometry by Lane & Muterspaugh (2004) was |
Lne2004 |
|
originally published as follows, but converted to BY, rho, and theta |
|
|
by WIH for inclusion in our catalogs: |
|
|
MJD dRA (arcsec) dDEC (arcsec) |
|
|
52862.30085 0.222109 +/- 0.000143 -0.119309 +/- 0.00000839 |
|
|
52863.28229 0.222233 +/- 0.000143 -0.119302 +/- 0.0000155 |
|
|
52864.31096 0.222134 +/- 0.000197 -0.119323 +/- 0.0000189 |
|
|
52865.29921 0.221981 +/- 0.000155 -0.119361 +/- 0.0000148 |
|
|
AB: Additional notes may be found in Wilson (1955). |
WRH1955 |
