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    UID:
    almahu_9949199518302882
    Format: XVIII, 294 p. , online resource.
    Edition: 1st ed. 2003.
    ISBN: 9789401707992
    Content: We stand at the threshold of an exciting era of Asteroseismology. In a few months' time, the Canadian small-satellite asteroseismology mission MOST will be laun­ ched. Danish and French missions MONS and COROT should follow, with the ESA mission Eddington following in 2007/8. Helioseismology has proved spec­ tacularly successful in imaging the internal structure and dynamics of the Sun and probing the physics of the solar interior. Ground-based observations have detected solar-like oscillations on alpha Centauri A and other 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 Hertzsprung-Russell diagram. For good reason it was decided to entitle our conference 'Asteroseismology Across the HR 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. In conceiving this meeting, the aim of the organisers was to facilitate a cross-fertilization of ideas and approaches between researchers working on different pulsators and with different areas of expertise. We venture to suggest that in this the conference was a great success.
    Note: Space 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.
    In: Springer Nature eBook
    Additional Edition: Printed edition: ISBN 9789048162413
    Additional Edition: Printed edition: ISBN 9781402011733
    Additional Edition: Printed edition: ISBN 9789401708005
    Language: English
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