| discov_num |
notes |
refcode |
| ISM 4 |
The Cepheid SU Cyg. This is also known as WRH 23Aa,Ab. The Wilson |
|
|
component were previously assigned to 19372+2920, but this was a |
|
|
position error on Wilson's part leading to the the pairs not being |
WRH1950a |
|
confirmed for many years. The wider components of Wilson will retain |
|
|
their historical, AE, AF, and AG component identifiers. The closer |
|
|
Aa,Ab pair will remain ISM 4. The problem was noted by Cliff |
|
|
Ashcraft and the correct system found by James Daley. |
|
|
Masses are 4.7 and 3.2 Msun. Estimated period = 1.5y, |
|
|
a = 2.6au = 0.003". |
Evs2013 |
| idgroup |
discov |
author |
| 1 |
ISM |
Ismailov, R.M. |
| 2 |
KRV |
Kervella, P., Thevenin, F., & Petr-Gotzens, M.G. |
| 11 |
KRV |
Kervella, P., Gallenne, A., Evans, N.R., Szabados, L., Arenouu, F., Merand, A., |
| 11 |
KRV |
Proto, Y., Karczmarek, P., Nardetto, N., Gieren, W. & Pietrzynski, G. |
| 12 |
KRV |
Kervella, P., Gallenne, A., Evans, N.R., Szabados, L., Arenouu, F., Merand, A., |
| 12 |
KRV |
Nardetto, N., Gieren, W. & Pietrzynski, G. |
| 14 |
KRV |
Kervella, P., Borgniet, S., de Souza, A.D., Merand, A., Gallenne, A., Rivinius, T., |
| 14 |
KRV |
Lacour, S., Carciofi, A., Faes, D.M., Le Bouquin, J.-B., Taormina, M., Pilecki, B., |
| 14 |
KRV |
Berger, J.-P., Bendjoya, P., Klement, R., Millour, F., Janot-Pacheco, E., Spang, A. |
