(Not yet in Simbad) | |
Write: | << NNNNNN>> << 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 |
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