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Asteroseismology Across the HR Diagram [E-Book] : Proceedings of the Asteroseismology Workshop Porto, Portugal 1–5 July 2002 /
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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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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):
Astronomy
Astrophysics.
Observations, Astronomical.
Physics.
Statistics.
Observations.
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  • Table of Contents
  • Description
  • Staff View

  • 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.

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