Talk:HD 126614

HD 126614 it's a triple star system and a NOT binary system

6. HD126614 A 6.1. Stellar Characteristics HD126614 (=HIP 70623) is identified in the Henry Draper and Hipparcos catalogs as a single star. As described in § 6.5, we directly detected by adaptive optics (AO) a faint M dwarf companion separated by 489mas from the bright primary. We refer to the bright primary star as HD126614A and the faint companion as HD126614B. These stars are unresolved in the Doppler and photometric variability observations described below. The planet announced below orbits HD126614A and is named HD126614Ab. In addition, HD126614A is orbited by a second M dwarf, NLTT37349, in a much wider orbit (Gould & Chanam´e 2004). This outer stellar companion is separated from HD126614A by 42"" and does not contaminate the Doppler or photometric observations

see at: http://exoplanets.org/papers/sixpack.pdf —Preceding unsigned comment added by 200.141.52.206 (talk) 14:30, 19 January 2010 (UTC)

I modified the article to trinary star system. BlueEarth (talk | contribs) 20:16, 19 January 2010 (UTC)