Spectroscopic diagnostics of pulsation in rotating stars

Thesis

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Titlepage

Table of Contents

1 General introduction

Part I Theory and Modeling

2 Observable characteristics of spheroidal modes

3 The diagnostic value of amplitude and phase diagrams derived from time series of spectra

4 On the alleged misidentification of tesseral modes

5 The effects of intrinsic profile variations on the IPS diagnostics

Part II Observations and Analyses

6 A new bright β Cephei star: β Lupi

7 Multi-periodic line-profile variability in the binary β Cep star v Centauri

8 Spectroscopic identifications of the non-radial pulsations in ε Centauri

9 A new bright β Cephei star: line-profile variability in ω¹ Scorpii

10 Non-radial pulsations in the O stars ξ Persei and λ Cephei

11 Inleiding en samenvatting

Dankwoord

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