Note sur le calcul numérique de pulsations stellaires

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1957

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Persée

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MESR

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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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Charles Allen Whitney et al., « Note sur le calcul numérique de pulsations stellaires », Bulletins de l'Académie Royale de Belgique, ID : 10.3406/barb.1957.68687


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The numerical integration of the pulsation equation is reduced to the resolution of a set of linear algebraic equations by considering the star as composed of discrete shells submitted to the appropriate pressure and gravity forces. The method has been applied to three models with encouraging results although further improvements are needed to reach the precision of standard numerical integration procedures.

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