| discov_num |
notes |
refcode |
| SEE 334 |
AB: lam Sco = 35 Sco = Shaula. Variable. Spectroscopic binary. |
|
| TNG 1 |
Aa,Ab: The combined solution orbit by Tango et al. (2006) determines |
Tng2006 |
|
component masses of 10.4 +/- 1.3 Msun and 8.1 +/- 1.0 Msun. There is |
|
|
also a pre-MS subcomponent to A with a mass of 1.8 +/- 0.2 Msun. The |
|
|
dynamical parallax is 112 +/- 5 mas, about a factor of two smaller |
|
|
than the Hipparcos value of 216 +/- 42. The dynamical value is much |
|
|
more accurate. Two components have calculated effective temperatures |
|
|
of 25000 +/- 1000 and 21000 +/- 1000 degrees Kelvin, respectively. |
|
|
Aa,Ab: Malkov et al. (2012) derive dynamical, photometric, and |
|
|
spectroscopic masses 77.47 +/- 30.56, 22.63, 10.96 Msun, respectively. |
Mlk2012 |
| refcode |
metd |
author |
reference |
| Mlk2012 |
not - |
Malkov, O.Yu., Tamazian, V.S., Docobo, J.A., & Chulkov, D.A. |
2012A&A...546A..69M |
| Mlk2012 |
|
A&A 546, A69, 2012 |
|
| Tng2006 |
Ks j |
Tango, W.J., Davis, J., Ireland, M.J., Aerts, C., Uytterhoeven, K., Jacob, A.P., |
2006MNRAS.370..884T |
| Tng2006 |
|
Mendez, A., North, J.R., et al. |
|
| Tng2006 |
|
MNRAS 370, 884, 2006 |
|
