Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-11-22
Astronomy and Astrophysics
Astrophysics
5 pages, 5 figures, to be published in 'Evolution of binary and multiple star systems', proceedings of conference, Bormio
Scientific paper
OAO1657-415 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 B6V or B5III star as a possible companion to the neutron star. We measure the observational parameters of the star and suggest reasons why OAO1657-415 may be unlike other high mass X-ray binaries.
Maxwell Diana H.
Norton Andrew J.
Roche Paul
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