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usic:chara_array_chara [2018/07/06 13:45] 127.0.0.1 external edit |
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- | {{/ | + | ====== CHARA Array ====== |
- | ====== | + | |
- | ====== Center for High Angular Resolution Astronomy ====== | + | {{: |
- | ==== [[http:// | + | |
- | ===== ===== | + | ====== Center for High Angular Resolution Astronomy |
- | \\ **Diameters of six M dwarfs** | + | |
+ | [[http:// | ||
+ | |||
+ | * Gravity darkening and oblateness of rapidly rotating main sequence stars. | ||
+ | * Pulsation and radial velocity projection factor in Cepheids. | ||
+ | * Hot exozodiacal dust around main sequence stars. | ||
+ | * Exoplanet stellar host diameters. | ||
+ | | ||
+ | | ||
+ | | ||
+ | * Images of a binary star system in eclipse. | ||
+ | * Precision stellar masses of spatially resolved spectroscopic binaries. | ||
+ | * Direct detection of high contrast companions around Cepheids, RS CVn, and Be stars. | ||
+ | | ||
+ | | ||
+ | | ||
+ | * Direct images | ||
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===== Overview of the CHARA Array ===== | ===== Overview of the CHARA Array ===== | ||
- | \\ Georgia State University’s Center for High Angular Resolution Astronomy (CHARA) operates an optical/ | + | |
+ | \\ Georgia State University’s Center for High Angular Resolution Astronomy (CHARA) operates an optical/ | ||
+ | |||
+ | The Beam Combining Laboratory (BCL) contains six beam combiners with complementary regimes of wavelength, sensitivity, measurement precision, and number of telescopes combined. The Array control system is capable of running | ||
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