| discov_num |
notes |
refcode |
| HDS3158 |
Cvetkovic et al. (2014) derive spectral types G4 and K3, masses 1.07 |
|
|
and 0.79 Msun. Dynamical parallax is 17.56 +/- 0.44 mas. |
Cve2014 |
|
A 111.1d spectroscopic solution for the B component has been found |
Tok2018d |
|
making this a triple system. |
|
|
Synthetic Spectrum gives Bt mags of 12.19 & 14.02 for Ba,Bb and 11.12 |
Mda2019 |
|
and 12.67 for Vt. The solution for the three components A, Ba and Bb |
|
|
Teff = 5836 +/- 80, 5115 +/- 80, and 4500 +/- 80, degrees Kelvin, |
|
|
R = 1.09 +/- 0.039, 0.596 +/- 0.05, and 0.49 +/- 0.06, \rsun, |
|
|
L = 1.24 +/- 0.10, 0.22 +/- 0.09, and 0.09 +/- 0.05, \lsun, |
|
|
M = 1.05 +/- 0.16, 0.83 +/- 0.16, and 0.67 +/- 0.16, \msun. |
|
| refcode |
metd |
author |
reference |
| Cve2014 |
orb - |
Cvetkovic, Z., Pavlovic, R., & Ninkovic, S. |
2014AJ....147...62C |
| Cve2014 |
|
AJ 147, 62, 2014 |
|
| Mda2019 |
orb j |
Masda, S.G., Docobo, J.A., Hussein, A.M., Mardini, M.K., Al-Ameryeen, H.A., Campo, |
2019AstBu..74..464M |
| Mda2019 |
+not |
P.P., Khan, A.R. & Pathan, J.M. |
|
| Mda2019 |
|
Astrophys. Bull. 74, 464, 2019 |
|
| Tok2018d |
orb j |
Tokovinin, A. |
2018AJ....156...48T |
| Tok2018d |
|
AJ 156, 48, 2018 |
|
