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HD 19467 System

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Exoplanetary Scratchpad

[SysBP Img]

A Yellow dwarf star with a faint T-dwarf companion. It is one of the most well studied brown dwarfs, first discovered using radial velocity in 1996. It was recently directly imaged, providing a benchmark for future exoplanet studies.

HD 19467 System Web PagesEdit

HD 19467 System In the NewsEdit

Dwarf Directly Imaged (Jan 2014)Edit

See AlsoEdit

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