Radio Astrometry of The Close Active Binary Hr 5110
The close active binary HR 5110 was observed at six epochs over 26 days using a global very long baseline interferometry array at 15.4 GHz. We used phase referencing to determine the position of the radio centroid at each epoch with an uncertainty significantly smaller than the component separation....
| Main Authors: | , , , |
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| Format: | Journal Article |
| Published: |
Institute of Physics Publishing
2015
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| Online Access: | http://hdl.handle.net/20.500.11937/69740 |