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δ Scuti Pulsations in Pre-main Sequence Stars

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Abstract

Intermediate mass pre-main sequence stars (1.5 to 5 M ⊙)cross the instability strip on their way to the main sequence.They are therefore expected to be pulsating in a similar way as the δScuti stars. In this review, I present the status of observational studies ofpulsations in these stars, and comment on prospects for futureinvestigations of these pulsations from the ground and from space.

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Authors and Affiliations

  1. Observatoire de Paris, LESIA, France

    Claude Catala

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  1. Claude Catala
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Catala, C. δ Scuti Pulsations in Pre-main Sequence Stars. Astrophysics and Space Science 284, 53–60 (2003). https://doi.org/10.1023/A:1023224326127

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  • DOI: https://doi.org/10.1023/A:1023224326127

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