Details on Acronym: [GKM2012] | |
| [GKM2012] | (Gvaramadze+Kniazev+Miroshnichenko+, 2012)= (WS) |
| Write: | <<[GKM2012] WSNN>> |
| N: | about 31 |
| Object: | (MIR) + Shell (SIMBAD class: MidIR = Mid-IR Source (3 to 30 µm)) |
| Note: | Circular shells, detected at 22µm in WISE archival data. In the format, WS stands for "WISE Shell". |
| Ref: | =2012MNRAS.421.3325G |
| by | GVARAMADZE V.V. , KNIAZEV A.Y., MIROSHNICHENKO A.S., BERDNIKOV L.N., LANGER N., STRINGFELLOW G.S., TODT H., HAMANN W.-R., GREBEL E.K., BUCKLEY D., CRAUSE L., CRAWFORD S., GULBIS A., HETTLAGE C., HOOPER E., HUSSER T.-O., KOTZE P., LOARING N., NORDSIECK K.H., O'DONOGHUE D., PICKERING T., POTTER S., ROMERO COLMENERO E., VAISANEN P., WILLIAMS T., WOLF M., REICHART D.E., IVARSEN K.M., HAISLIP J.B., NYSEWANDER M.C., LACLUYZE A.P. |
| Mon. Not. R. Astron. Soc., 421, 3325-3337 (2012) | |
| Discovery of two new Galactic candidate luminous blue variables with Wide-field Infrared Survey Explorer. | |
| o | Figs 1-2, Tables 3-4: <[GKM2012] WSN> (Nos WS1-WS2). |
| Ref: | =2017ASPC..508..207G |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: WS | |
| WS | (WISE Shell) |
| ***** | Avoid the usage of WS, prefer [GKM2012] |
| Origin | of the Acronym: A = Assigned by the author(s) |