Details on Acronym: [WCB2018] | |
| [WCB2018] | (Williams+Canton+Bellini+, 2018) |
| Write: | <<[WCB2018] NNNNNN>> <<[WCB2018] WDNN>> |
| N: | 52+33 |
| Object: | Poss. WD + WD (SIMBAD class: Unknown = Object of Unknown Nature) |
| Stat: | is completely incorporated in Simbad |
| Note: | MMT Megacam imaging and Keck I LRIS spectroscopy of N=52 white dwarf candidates, including N=33 confirmed white dwarfs (format WDNN), in the open star cluster M67. |
| in source: | NGC 2682 = M 67 |
| Ref: | =2018ApJ...867...62W |
| by | WILLIAMS K.A. , CANTON P.A., BELLINI A., BOLTE M., RUBIN K.H.R., GIANNINAS A., KILIC M. |
| Astrophys. J., 867, 62-62 (2018) | |
| Ensemble properties of the white dwarf population of the old, solar metallicity open star cluster Messier 67. | |
| o | Table 3, col(Object ID): <[WCB2018] NNNNNN> N=52 among (2231-292440). Table 5, col(Alias): <[WCB2018] WDNN> (Nos WD1-WD33). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |