Datatype: smi
The datatype smi refers to a photometric system designed to
observe Wolf-Rayet stars and avoid the strong emission-lines. A few clusters
containing Wolf-Rayet stars have been observed in this system.
Record structure
| No | : | Star number |
|---|
| Ref | : | Data source |
|---|
| v | : | v magnitude |
|---|
| b-v | : | b-v colour index |
|---|
| u-b | : | u-b colour index |
|---|
| N | : | Number of measurements |
|---|
Database access
List of clusters
Query the references
Jean-Claude.Mermilliod@obs.unige.ch
Last Update: 17 February 1998