Omega Orionis and the Be stars.

We summarize the results of a multisite spectroscopic and photometric campaign on the Be star omega Orionis. There is only one period, P = 0.97d, which is visible in the photometry and line profile variations. We caution against the indiscriminate use of the radial velocity to infer multiperiodicity...

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Bibliographic Details
Main Authors: Balona, L. A., Handler, G., Aerts, C., Bozic, H., Guinan, E. F., James, D. J., Kaye, A. B., Shobbrook, R. R.
Format: Villanova Faculty Authorship
Language:English
Published: 2002
Online Access:http://ezproxy.villanova.edu/login?url=https://digital.library.villanova.edu/Item/vudl:176541