Gaia's detection of eclipsing binaries - explained

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Published for Gaia Data Release 3 on 13 June 2022.

Top panel: Light curve, i.e. the flux seen by the observer as the sum of
the contributions from each element of the stars' surfaces.
Bottom-left panel: Simulated plane-of-sky view (in "false" colours).
Bottom-right panel: Discrete grids that represent the stars' surfaces.
Colour palettes indicate the temperature differences (with respect to each
star's effective temperature) due to gravity and mutual heating.

-- Additional information (simulation parameters) --
* Eccentricity: 0
* Inclination: 83.08 (degrees)
* Period: 8.93562 (days)
* Mass ratio (M2 / M1): 0.5
* Effective temperatures:
* t1 = 4500 (K)
* t2 = 7000 (K)
* Roche fill factors:
* s1 = 0.98
* s2 = 0.7

Acknowledgements: ESA/Gaia/DPAC/CU4/NSS, G. Sadowski, A. Jorissen, C. Siopis
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Do these stars really orbit that close? The deformation is stunning. Does this affect stability of convection cells and star activity?

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