Short period line profile and light variations in the Be star Orionis.

We present the results of a multisite spectroscopic and photometric campaign on the Be star ω Orionis. From the photometry and radial velocity variation of several spectral lines, we confirm that the star is a variable with period P=0.97d. Only one period can be extracted from both the photometric a...

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Bibliographic Details
Main Authors: Balona, L. A., Aerts, C., Bozic, H., Guinan, E. F., Handler, G., James, D. J., Kaye, A. B., Shobbrook, R. R.
Format: Villanova Faculty Authorship
Language:English
Published: 2001
Online Access:http://ezproxy.villanova.edu/login?url=https://digital.library.villanova.edu/Item/vudl:176556