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AB Doradus System

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Exoplanetary Scratchpad

[SysBP Img]

Nearby triple star system. The very dim star C was resolved with a technique that will next be used to attempt to resolve exoplanets. This found that it was a very dim red dwarf instead of a brown dwarf, and is one of the lowest mass stars known. Principle star of the AB Doradus Moving Group.Nearby triple star system. The very dim star C was resolved with a technique that will next be used to attempt to resolve exoplanets. This found that it was a very dim red dwarf instead of a brown dwarf, and is one of the lowest mass stars known. Principle star of the AB Doradus Moving Group.

AB Doradus Web PagesEdit

AB Doradus System In the NewsEdit

Dim Star Used As a Testbed for New Exoplanet Detection Technique (June 2007)Edit

http://physicsweb.org/articles/news/11/6/14/1
http://cordis.europa.eu/fetch?CALLER=EN_NEWS&ACTION=D&SESSION=&RCN=27954

See AlsoEdit

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