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Cited article:

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THE ROLE OF θ OPH IN THE FORMATION AND EVOLUTION OF THE PIPE NEBULA—IS STAR FORMATION EVER ISOLATED?

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Seismic modelling of OB stars

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Proceedings of the International Astronomical Union 6 (S272) 457 (2010)
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Modelling results for two late Be stars observed by CoRoT

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Astronomische Nachrichten 331 (9-10) 1061 (2010)
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