| C1900.0 | : | 23138-1400 |
|---|---|---|
| C2000.0 | : | 231906668-13273079 |
| Comp. | : | A |
| Magn. | : | 5.21(V) |
| Spect. | : | G5IV ; K2V |
| ADS 16672 | BD -14 6448 | Flamsteed 94 Aqr | GAIADR2 2411855072801158656 |
| GAIADR3 2411855072801158656 | GJ 894.2 | HD 219834 | HIP 115126 |
| HR 8866 |
| Element | Value | Std. dev. | |
|---|---|---|---|
| Period (d.) | : | 2323.6 | |
| T0 (xJD-2,400,000.0) | : | 29308.4 | |
| Reference T0/epoch | : | JD | |
| Eccentricity | : | 0.08 | |
| omega primary (deg.) | : | 225.7 | |
| K1 (km/s) | : | 5.5 | |
| K2 (km/s) | : | ||
| V0 (km/s) | : | +10.8 | |
| sigma residuals primary | : | ||
| sigma residuals secondary | : | ||
| #RV primary | : | ||
| #RV secondary | : | ||
| Grade | : | 2.0 | |
| Contributor | : | DAO | |
| Status | : | PUB | |
| Bibcode | : | 1962ApJ...135..301S | |
| Derived quantities (on the fly, from the above quantities) | |||
| a1sini (km) | : | 1.75172e+08 | 0 |
| f(m) (sol.mass) | : | 0.0398225 | 0 |
The epoch is T0. Sarma notes that the probable error of a single velocity (1.2 km/s) is large for spectrograms of this type of star obtained with the Mills spectrograph, and he suggests some additional cause of velocity variation may be acting. Lucy & Sweeney adopt a circular orbit. The star is the brighter member of A.D.S. 16672: B is 7.5m at 13.0" and shares the proper motion of A.
