| discov_num |
notes |
refcode |
| STT 596 |
iot Peg = 24 Peg. The primary is a spectroscopic binary. |
|
|
Optical pair, based on study of relative motion of the components |
|
|
using the method of apparent motion parameters. |
Kiy2008 |
| PTI 1 |
SB2. Combined solution by Boden et al. (1999), including visibilities |
Bod1999a |
|
from the Palomar Testbed Interferometer, plus spectroscopy. Authors |
|
|
give two very similar solutions, made using two data sets. Values were |
|
|
averaged in the orbit catalog. |
|
|
See also discussion of iot Peg system by Morel et al. (2000). |
Mrl2000 |
|
Combined spectroscopic/astrometric solution, based on high-resolution |
|
|
echelle spectra plus archival PTI visibility measurements. |
|
|
Derived masses 1.33249 +/- 0.00086 and 0.83050 +/-0.00055 Msun, |
|
|
distance 11.534 +/- 0.019 pc. |
Knc2010 |
|
Malkov et al. (2012) derive dynamical, photometric, and spectroscopic |
|
|
masses of 2.27 +/- 4.55, 2.36, and 1.20 Msun, respectively. |
Mlk2012 |
| refcode |
metd |
author |
reference |
| Bod1999a |
orb - |
Boden, A.F., Koresko, C.D., van Belle, G.T., Colavita, M.M., Dumont, P.J., |
1999ApJ...515..356B |
| Bod1999a |
|
Gubler, J., Kulkarni, S.R., Lane, B.F., et al. |
|
| Bod1999a |
|
ApJ 515, 356, 1999 |
|
| Kiy2008 |
- |
Kiyaeva, O.V., Kiselev, A.A. & Izmailov, I.S. |
2008SvAL...32..405K |
| Kiy2008 |
|
SvAL 34, 405, 2008 |
|
| Knc2010 |
orb - |
Konacki, M., Muterspaugh, M.W., Kulnarni, S.R., & Helminiak, K.G. |
2010ApJ...719.1293K |
| Knc2010 |
|
ApJ 719, 1293, 2010 |
|
| Mlk2012 |
not - |
Malkov, O.Yu., Tamazian, V.S., Docobo, J.A., & Chulkov, D.A. |
2012A&A...546A..69M |
| Mlk2012 |
|
A&A 546, A69, 2012 |
|
| Mrl2000 |
- |
Morel, P.J., Morel, Ch., Provost, J., & Berthomieu, G. |
2000A&A...354..636M |
| Mrl2000 |
|
A&A 354, 636, 2000 |
|
