| discov_num |
notes |
refcode |
| BU 1240 |
26 Aur. Composite spectrum; B9.5V+F9III. Light variability suspected. |
|
|
See Baize & Petit (1989) catalog of doubles with variable component. |
Baz1989d |
|
Only elements P and T have been amended by Starikova (1977) from the |
Sta1977a |
|
orbit of Baize (1956). |
Baz1956 |
|
Romero (2008) estimates masses of the A and B components as 2.1 +/- |
FMR2008 |
|
1.0 and 3.0 +/- 0.4 Msun, respectively; spectral types are G8III and |
|
|
A1IV or B9.5V. |
|
|
AB: Malkov et al. (2012) derive dynamical, photometric, and |
|
|
spectroscopic masses 6.87 +/- 22.98, 5.45, and 4.82 Msun, respectively. |
Mlk2012 |
| STF 753 |
Romero (2008) analyzes the optical/physical nature of the C component; |
FMR2008 |
|
the spectral is determined to be about A6V and it appears to be |
|
|
gravitationally bound to the AB pair, with an estimated orbital period |
|
|
of ~46,000 years. |
|
|
AB,C: H 3 64. |
MEv2010 |
| BU 90 |
Romero (2008) derives a proper motion for D (+0.4 +/- 2.1 mas/yr in |
FMR2008 |
|
RA, -12.6 +/- 1.6 mas/yr in Dec) based on that of the AB pair plus the |
|
|
relative motion of AB,D between the years 1856 and 2002. He also |
|
|
concludes that D is optical, with a spectral type estimated at K1III |
|
|
and distance of ~870pc (both determinations corrected for reddening). |
|
