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Encyclopedia > Contact binary

Contact binaries are a type of binary stars where both components of the binary fill their Roche lobes. The uppermost part of the stellar atmospheres forms a common envelope that surrounds both stars. As the friction of the envelope brakes the orbital motion, the stars coalesce in the future, unless something dramatic happens. Example: W UMa


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Eclipsing Binaries with MONS (875 words)
Particular aspects of eclipsing binaries are studied within the context of MONS (eccentric systems, systems with pulsating components, second order light curve effects).
The most interesting fact about eclipsing binaries is that all kinds of stars are found as members of binaries: from normal main sequence stars, variable stars, evolved giants and supergiants, to collapsed objects.
The main asset of MONS with respect to eclipsing binaries is its capability of obtaining stable, long time series photometry of moderately bright stars with millimagnitude-level accuracy.
ESA Science & Technology: Binary Stars (874 words)
Resolved binaries will be studied in different populations of stars: nearby star-forming regions, open clusters and associations as well as field binaries of different ages.
Large fractions of astrometric binaries with periods in the range 0.03 to 30 years will be immediately recognized by their poor fit to the standard 5 parameter single star astrometric model.
The surprising number of new eclipsing and contact binaries discovered by Hipparcos at magnitudes as bright as 7 mag demonstrates that even bright binary systems are not well surveyed.
  More results at FactBites »


 
 

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