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Published byLindsey Nichols Modified over 9 years ago
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Time Domain Astrophysics in South Africa 2 Astero-seismology
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Monitoring Time variations in intrinsic variables in order to infer their properties such as mass, luminosity, rotation rate, internal composition
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Seismic Waves trapped in Stars Stars pulsate according to y=A n ( r ) Y lm (theta, phi) exp(-omega t) Where n l m describe a mode A good start to astero-seismology is in determining these for as many modes as possible
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Probing a star with seismic waves
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Asteroseismology Research in South Africa Observational Studies include - mode identification using photometry alone (determines l) - mode identification using Baade-Wesselink methods (combination) - mode-identification by observing line profile variations On roAp stars, delta Scuti, sdB stars, beta Cepheid etc
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Search for new Pulsating stars Rapidly Oscillating Ap stars (SAAO) 5 min < P puls <16 min
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Frequency Spectrum dipole(-like) like nothing you have ever seen new, improved mode strange doublet
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Pulsating sdB stars hot Horizontal Branch stars with temperatures of about 30,000 K Periods 2 -3 minutes
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Observational Facilities Photo-electric photometers CCDs (also have frame-transfer) Giraffe spectrograph {R = 39000, wavelength 3820 - 9240 angstrom, V < 9} SALT ?
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Theory Non-linear theory (SAAO) Radiative Transfer and Oscillations in A stars (UCT/SAAO)
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