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...
Main Authors: | , , , , , , , |
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Format: | |
Language: | English |
Published: |
2001
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Online Access: | http://ezproxy.villanova.edu/login?url=https://digital.library.villanova.edu/Item/vudl:176556 |