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Paper: PAVO@CHARA High Angular Resolution Observations of Rapid Rotators
Volume: 465, Four Decades of Massive Star Research - A Scientific Meeting in Honor of Anthony J. Moffat
Page: 95
Authors: Maestro, V.; Huber, D.; Ireland, M.; Tuthill, P.
Abstract: Stellar rotation distorts the stellar spherical shape assumed in simplistic stellar models. We present first results of a study of a small sample of bright (V < 4), compact (size < 0.8 mas), fast rotators (V sin i > 150 km s-1). We have measured the projected oblateness of four of these stars using interferometric high angular resolution observations, deriving a lower bound for the rotational to break-up velocity ratio.
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