Measuring V-rot sin i in post common envelope binaries
We determine the projected rotational velocities, V-rot sin i of the secondary stars in the PCEBs EG UMa, PG1026+002, REJ2013+400 and GD123. We find that the results are inconsistent with the values expected from other information we have about the binaries, particularly when V-rot sin i is measured...
| Main Authors: | , , , , |
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| Format: | Conference item |
| Published: |
2001
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