RS Canum Venaticorum
E1988457
UNEXPLORED
RS Canum Venaticorum is the prototype of a class of close binary stars characterized by strong chromospheric activity and periodic brightness variations driven by large starspots and magnetic phenomena.
All labels observed (1)
| Label | Occurrences |
|---|---|
| RS Canum Venaticorum canonical | 1 |
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.