The wind-collision region of HD 93129A from LBA observations (original) (raw)

2007

Abstract

The O2 If* star HD 93129A, the brightest member of the Tr 14 cluster in Carina, has recently been observed as a strong non-thermal radio emitter (Benaglia & Koribalski 2005, C678), with a 1.4 GHz flux of ~10 mJy. Also recently, Nelan et al. (2004) using FGS-HST data, have demonstrated that this star has an O-star companion 55 mas distant

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