OA01657-415: A 'Missing link' in high-mass X-ray binaries?
OA01657-415 is only the seventh eclipsing X-ray pulsar known and therefore has the potential to yield only the seventh mass of a neutron star in an X-ray binary. Here we report photometric and spectroscopic observations of candidates for the optical counterpart to the system and identify a B5III or...
Main Authors: | , , |
---|---|
Format: | Conference item |
Izdano: |
2001
|