Asteroseismology for the nonspecialist /

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"Version: 20251101"--Title page verso.Includes bibliographical references.1. A brief review of stellar structure and evolution -- 1.1. Internal stellar conditions -- 1.2. Stellar timescales -- 1.3. Equations of stellar structure -- 1.4. Radiation transfer and opacity -- 1.5. Convective transport -- 1.6. Calculating stellar models -- 1.7. Stellar evolution -- 1.8. Model comparisons2. An observational perspective -- 2.1. Upper main sequence stars -- 2.2. Lower main sequence stars -- 2.3. Pre-MS stars -- 2.4. Evolved stars -- 2.5. White dwarfs -- 2.6. Classical pulsators3. The physics of stellar oscillations -- 3.1. Mathematical preludes -- 3.2. Oscillations -- 3.3. Conservation laws -- 3.4. Important frequencies -- 3.5. Types of waves -- 3.6. The stellar oscillation equations -- 3.7. The physical interpretation of oscillation modes -- 3.8. Mode inertia -- 3.9. Excitation and damping4. Data reduction tools and techniques -- 4.1. Oscillation frequencies -- 4.2. Spatial response -- 4.3. Photometry -- 4.4. Spectroscopy5. Data analysis tools and techniques -- 5.1. Fourier analysis -- 5.2. Aliasing and Nyquist sampling -- 5.3. Noise sources and effects -- 5.4. Gaps and uneven sampling -- 5.5. Lomb-Scargle periodogram6. From frequencies to physics : basic topics -- 6.1. Measuring the power spectrum -- 6.2. Average seismic parameters -- 6.3. Echelle diagrams -- 6.4. Massive stars -- 6.5. Evolved stars -- 6.6. Forward modeling7. Uncertainties and limitations -- 7.1. Global asteroseismic parameters : scaling relations -- 7.2. Choosing significance criteria -- 7.3. Estimating uncertainties in measured parameters -- 7.4. Surface effect -- 7.5. Estimating uncertainties in physical parameters8. From frequencies to physics : an introduction to advanced topics -- 8.1. Frequency inversions and the inverse problem -- 8.2. Rotation -- 8.3. Magnetic fields -- 8.4. Glitches -- 8.5. Mode identification -- 8.6. Machine learning.Full-text restricted to subscribers or individual document purchasers.This book outlines the physics behind stellar oscillations and the information they encode about stellar structure, and summarizes the current state of the art in the field. It also describes commonly-used data reduction and analysis techniques and tools for asteroseismology, and discusses the uncertainties and limitations of both oscillation frequency measurements and the physical parameters derived from them. An introduction to some advanced topics, such as measurements of rotation and magnetic fields, is also included. The focus of the book is on the successful application, use, and physical interpretation of asteroseismology by nonspecialists in the field. It is aimed at professional and future professional astronomers at all levels from advanced undergraduate on up.Professional astronomers who wish use asteroseismic analyses without being specialists in the area.Also available in print.Mode of access: World Wide Web.System requirements: Adobe Acrobat Reader, EPUB reader, or Kindle reader.Derek Buzasi received his BA in Physics at the University of Chicago and his PhD in Astronomy at Pennsylvania State University. He has worked at a variety of institutions, including the National Center for Atmospheric Research, Johns Hopkins University, the California Institute of Technology, and the University of California at Berkeley, and served on the science team for NASA's Kepler mission. Since January 2025, he has been a Professor in the Department of Astronomy and Astrophysics at the University of Chicago.Title from PDF title page (viewed on December 1, 2025).

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Series Title

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Call Number

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Publisher

: .,

Collation

1 online resource (various pagings) :illustrations (some color).

Language

English

ISBN/ISSN

9780750356336

Classification

523.8

Content Type

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Media Type

-

Carrier Type

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Edition

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Subject(s)

Galaxies & stars.
Astroseismology.
SCIENCE / Space Science / Stellar & Solar.

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Statement of Responsibility

Derek L. Buzasi.

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