AG Carinae: a Luminous Blue Variable with a High Rotational Velocity

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Scientific paper

We report the detection of broad absorptions due to Si IV λλ4088--4116 in the luminous blue variable (LBV) AG Carinae during its last hot phase (2001-2003). Our NLTE spectral analysis, with the radiative transfer code CMFGEN, revealed the photospheric nature of these lines. Using a recently developed code to compute synthetic spectra in 2D geometry allowing for the effects of rotation, we could match the broad absorptions observed in the 2001 April spectrum with a high projected rotational velocity of 190 ± 30 km/s. Our results show direct spectroscopic evidence, for the first time, that an LBV may rotate at a significant fraction of its break-up velocity. Thus, AG Car (and possibly other LBVs) is indeed close to the ΓΩ limit, as predicted by theoretical studies of LBVs.

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