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- W2108676022 abstract "Abstract While theoretical studies have long suggested a fast-rotating nature of Luminous Blue Variables (LBVs), observational confirmation of fast rotation was not detected until recently. Here I discuss the diagnostics that have allowed us to constrain the rotational velocity of LBVs: broadening of spectral lines and latitude-dependent variations of the wind density structure. While rotational broadening can be directly detected using high-resolution spectroscopy, long-baseline near-infrared interferometry is needed to directly measure the shape of the latitude-dependent photosphere that forms in a fast-rotating star. In addition, complex 2-D radiative transfer models need to be employed if one's goal is to constrain rotational velocities of LBVs. Here I illustrate how the above methods were able to constrain the rotational velocities of the LBVs AG Carinae, HR Carinae, and Eta Carinae." @default.
- W2108676022 created "2016-06-24" @default.
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- W2108676022 date "2010-07-01" @default.
- W2108676022 modified "2023-09-25" @default.
- W2108676022 title "Effects of fast rotation on the wind of Luminous Blue Variables" @default.
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- W2108676022 doi "https://doi.org/10.1017/s1743921311009975" @default.
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