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Pré-Publication, Document De Travail Année : 2010

Spectro-interferometric observations of interacting massive stars with VEGA/CHARA

Daniel Bonneau
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Denis Mourard
Philippe Stee

Résumé

We obtained spectro-interferometric observations in the visible of $\beta$~Lyrae and $\upsilon$~Sgr using the instrument VEGA of the CHARA interferometric array. For $\beta$~Lyrae, the dispersed fringe visibilities and differential phases were obtained in spectral regions containing the H$\alpha$ and HeI 6678 lines and the H$\beta$ and HeI 4921 lines. Whereas the source is unresolved in the continuum, the source of the emission lines is resolved and the photocenter of the bulk of the H$\alpha$ emission exhibits offsets correlated with the orbital phase. For $\upsilon$~Sgr, both the continuum and H$\alpha$ sources are resolved, but no clear binary signal is detected. The differential phase shift across the line reveals that the bulk of the H$\alpha$ emission is clearly offset from the primary.
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Dates et versions

hal-00432349 , version 1 (05-01-2010)

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Daniel Bonneau, Olivier Chesneau, Denis Mourard, Philippe Stee. Spectro-interferometric observations of interacting massive stars with VEGA/CHARA. 2010. ⟨hal-00432349⟩
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