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      Revisiting the rigidly rotating magnetosphere model for σ Ori E – II. Magnetic Doppler imaging, arbitrary field RRM, and light variability★

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          Most cited references 33

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          Radiation-driven winds in Of stars

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            Non-LTE line-blanketed model atmospheres of hot stars. 1: Hybrid complete linearization/accelerated lambda iteration method

             T Lanz,  I. Hubeny (1995)
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              A computer program for calculating non-LTE model stellar atmospheres

               I. Hubeny (1988)
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                Author and article information

                Journal
                Monthly Notices of the Royal Astronomical Society
                Oxford University Press (OUP)
                1365-2966
                0035-8711
                August 01 2015
                August 01 2015
                : 451
                : 2
                : 2015-2029
                Article
                10.1093/mnras/stv1086
                © 2015

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