Asteroseismology Across the HR Diagram [E-Book] : Proceedings of the Asteroseismology Workshop Porto, Portugal 1–5 July 2002 / edited by Michael J. Thompson, Margarida S. Cunha, Mário J. P. F. G. Monteiro.
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 ha...
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Full text |
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Personal Name(s): | Cunha, Margarida S., editor |
Monteiro, Mário J. P. F. G., editor / Thompson, Michael J., editor | |
Imprint: |
Dordrecht :
Springer,
2003
|
Physical Description: |
XVIII, 294 p. online resource. |
Note: |
englisch |
ISBN: |
9789401707992 |
DOI: |
10.1007/978-94-017-0799-2 |
Subject (LOC): |
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245 | 1 | 0 | |a Asteroseismology Across the HR Diagram |h [E-Book] : |b Proceedings of the Asteroseismology Workshop Porto, Portugal 1–5 July 2002 / |c edited by Michael J. Thompson, Margarida S. Cunha, Mário J. P. F. G. Monteiro. |
246 | 3 | |a Proceedings of the Asteroseismology Workshop, held in Porto, Portugal, 1-5 July 2002 | |
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505 | 0 | |a 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. | |
520 | |a 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. | ||
650 | 0 | |a Astronomy |x Observations. | |
650 | 0 | |a Astrophysics. | |
650 | 0 | |a Observations, Astronomical. | |
650 | 0 | |a Physics. | |
650 | 0 | |a Statistics. | |
700 | 1 | |a Cunha, Margarida S., |e editor | |
700 | 1 | |a Monteiro, Mário J. P. F. G., |e editor | |
700 | 1 | |a Thompson, Michael J., |e editor | |
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