Keywords
Beta CMa Stars:Spectroscopy
Beta CMa Stars:Velocity Curves
Spectroscopy:Beta CMa Stars
Beta CMa Stars:Velocity Curves
Spectroscopy:Beta CMa Stars
How to Cite
The behaviour of the atmosphere of σ Scorpii. (1985). Revista Mexicana De Astronomía Y Astrofísica, 10(1), 293-305. https://astronomia.unam.mx/journals/rmxaa/article/view/1985rmxaa..10..293c
Abstract
The β CMa star σ Scorpii has been observed spectroscopically along two cycles. It has been found that absorption lines representing different depths in the atmosphere (excluding the transition region) yield different radial velocity curves; the amplitudes decrease and the γ's become more negative in the outermost layers. Ca II λ3933 Å has a chromospheric component.Similar Articles
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