Sobolev type line profiles in case of wind density perturbations modulated by non radial pulsations

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1986

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Copyright PERSEE 2003-2023. Works reproduced on the PERSEE website are protected by the general rules of the Code of Intellectual Property. For strictly private, scientific or teaching purposes excluding all commercial use, reproduction and communication to the public of this document is permitted on condition that its origin and copyright are clearly mentionned.



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Richard Scuflaire et al., « Sobolev type line profiles in case of wind density perturbations modulated by non radial pulsations », Bulletins de l'Académie Royale de Belgique, ID : 10.3406/barb.1986.57633


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We have studied the modifications induced on the P Cygni line profiles of an outwards accelerating wind by density fluctuations modulated by non radial pulsations.

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