| discov_num |
notes |
refcode |
| COO 157 |
A semiregular variable, V766 Cen. |
|
| CSU 1 |
Aa,Ac: Chesneau et al. (2014) imaged a close companion to the |
|
|
supergiant V766 Cen, using VLTI/AMBER. Based on visual photometry, |
|
|
they estimate the orbital period at 1304 +/- 6d. |
Csu2014 |
|
Wittkowski et al (2017) used VLTI/PIONIER for followup H-band imaging. |
|
|
At the 2014 epoch they believe the companion was behind the primary. |
|
|
They conclude the companion is most likely a cool giant or supergiant |
|
|
with a mass ~5 Msun. |
Wtk2017 |
| refcode |
metd |
author |
reference |
| Csu2014 |
A j |
Chesneau, O., Meilland, A., Chapellier, E., Millour, F., van Genderen, A.M., |
2014A&A...563A..71C |
| Csu2014 |
|
Naze, Y., Smith, N., Spang, A., Smoker, J.V., Dessart, L., Kanaan, S., |
|
| Csu2014 |
|
Bendjoya, Ph., et al. |
|
| Csu2014 |
|
A&A 563, A71, 2014 |
|
| Wtk2017 |
K - |
Wittkowski, M., Abellan, F.J., Arroyo-Torres, B., Chiavassa, A., Guirado, J.C., |
2017A&A...606L...1W |
| Wtk2017 |
|
Marcaide, J.M., Alberdi, A., de Wit, W.J., Hofmann, K.-H., Meilland, A., |
|
| Wtk2017 |
|
Millour, F., Mohamed, S., & Sanchez-Bermudez, J. |
|
| Wtk2017 |
|
A&A 606, L1, 2017 |
|
