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OverviewGround-based observations have detected solar-like oscillations on Sun-like stars, and diagnostics similar to those used in helioseismology are now being used to test and constrain the physics and evolutionary state of these stars. Multi-mode oscillations are being observed in an abundance of other stars, including slowly pulsating B stars (SPB stars), delta-Scuti stars, Ap stars and the pulsating white dwarfs. New classes of pulsators continue to be discovered across the Herzsprung-Russell diagram. Yet the challenges still to be faced to make asteroseismology across the HR diagram a reality are formidable. Observation, data analysis and theory all pose hard problems to be overcome. This book aims to facilitate a cross-fertilisation of ideas and approaches between fields covering different pulsators and with different areas of expertise. It covers most known types of pulsators, reflecting a productive and far-reaching interchange of ideas, which should make it a useful reference for researchers and postgraduate students working on stellar structure and evolution. Full Product DetailsAuthor: Michael J. Thompson , Margarida S. Cunha , Mário J.P.F.G. MonteiroPublisher: Springer-Verlag New York Inc. Imprint: Springer-Verlag New York Inc. Edition: 2003 ed. Dimensions: Width: 15.50cm , Height: 1.90cm , Length: 23.50cm Weight: 1.370kg ISBN: 9781402011733ISBN 10: 1402011733 Pages: 294 Publication Date: 31 May 2003 Audience: College/higher education , Professional and scholarly , Postgraduate, Research & Scholarly , Professional & Vocational Format: Hardback Publisher's Status: Active Availability: In Print ![]() This item will be ordered in for you from one of our suppliers. Upon receipt, we will promptly dispatch it out to you. For in store availability, please contact us. Table of ContentsSpace and Ground Based Data for Asteroseismology.- STARE Results on a Single Field: Tens of New Pulsating Stars.- The Eddington Mission.- Present Observational Status of Solar-Type Stars.- Present Observational Status of the Intermediate Mass Stars.- Present Observational Status of High Mass Pulsating Stars.- Old Pulsators: White Dwarfs and their Immediate Precursors.- ? Scuti Pulsations in Pre-Main Sequence Stars.- Solar-like Oscillations in Semiregular Variables.- Discovery of a New Class of Pulsating Stars: Gravity Mode Pulsators among Subdwarf B Stars.- Recent Observations of PMS ? Scuti Stars.- Multicolour Photometry for Mode Identification.- High-Resolution Spectroscopy for Mode Identification.- Theoretical Clues for Mode Identification — Instability Ranges and Rotational Splitting Patterns.- Peakbagging for Solar-Like Stars.- Mode Identification from Line Profiles Using the Direct Fitting Technique.- Statistical Revision of the Moment Method.- An Improved Method of Photometric Mode Identification: Applications to Slowly Pulsating B, ? Cephei, ? Scuti and ? Doradus Stars.- Photometric Nonadiabatic Observables in Rotating ß Cephei Models.- Gravity Modes in Delta Scuti Stars.- Seismic Inference Using Genetic Algorithms.- Stellar Inversions.- On the Principal Asteroseismic Diagnostic Signatures.- Diagnostics of the Internal Structure of Stars Using the Differential Response Technique.- Stellar Convection.- Mixing and Diffusion in Stars.- Are Pulsation and Magnetic Axes Aligned in roAp Stars?.- Seismic Diagnostics of Stellar Convection Treatment from Oscillation Amplitudes of p-Modes.- Of Variability, or its Absence, in HgMn Stars.- A Study of the Solar-Like Properties of ? Hydri.- Giant Vibrations in Dip.- Stochastic Excitation of Gravity Waves by Overshooting Convection in Solar-Type Stars.- p-Mode Oscillations of ? Cen A.- Outstanding Issues for the Pulsation of Young Stars.- Outstanding Issues for Post-Main Sequence Evolution: Instability Strips and Excitation of Modes in Compact Pulsators.- Hot Subdwarfs: Magnetic, Oscillatory and other Physical Properties.- Nonlinearity of Nonradial Modes in Evolved Stars.- Summary: Problems, Connections and Expectations.ReviewsAuthor InformationTab Content 6Author Website:Countries AvailableAll regions |