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Related papers: Asteroseismology: Data Analysis Methods and Interp…

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The seismic study of the Sun and other stars offers a unique window into the interior of these stars. Thanks to helioseismology, we know the structure of the Sun to admirable precision. In fact, our knowledge is good enough to use the Sun…

Solar and Stellar Astrophysics · Physics 2016-10-19 Sarbani Basu

Asteroseismology has the capability of delivering stellar properties which would otherwise be inaccessible, such as radii, masses and thus ages of stars. When this information is coupled with classical determinations of stellar parameters,…

Solar and Stellar Astrophysics · Physics 2019-08-14 Luca Casagrande , Victor Silva Aguirre , Aldo M. Serenelli , Dennis Stello , Sofia Feltzing , Katharine J. Schlesinger

We describe three useful applications of asteroseismology in the context of exoplanet science: (1) the detailed characterisation of exoplanet host stars; (2) the measurement of stellar inclinations; and (3) the determination of orbital…

Asteroseismology, the study of stellar pulsations, offers insights into the internal structures and evolution of stars. Analysing the variations in a star's brightness allows the determination of fundamental properties such as mass, radius,…

Instrumentation and Methods for Astrophysics · Physics 2024-06-12 Mathias Michielsen

Massive stars are important metal factories in the Universe. They have short and energetic lives, and many of them inevitably explode as a supernova and become a neutron star or black hole. In turn, the formation, evolution and explosive…

Solar and Stellar Astrophysics · Physics 2020-08-26 Dominic M. Bowman

The study of fundamental properties (such as temperatures, radii, masses, and ages) and interior processes (such as convection and angular momentum transport) of stars has implications on various topics in astrophysics, ranging from the…

Solar and Stellar Astrophysics · Physics 2016-04-27 Daniel Huber

These notes were originally prepared as additional material for the lessons I have given at the summer school Gamma-ray Astrophysics and Multifrequency: Data analysis and astroparticle problems, organized by the Department of Physics of the…

Instrumentation and Methods for Astrophysics · Physics 2009-10-13 Luigi Foschini

Asteroseismology using space-based telescopes is vital to our understanding of stellar structure and evolution. {\textit{CoRoT}}, {\textit{Kepler}}, and {\textit{TESS}} space telescopes have detected large numbers of solar-like oscillating…

Solar and Stellar Astrophysics · Physics 2021-05-12 Z. Çelik Orhan , M. Yıldız , C. Kayhan

Recent developments in instrumentation (e.g., in particular the Kepler and CoRoT satellites) provide a new opportunity to improve the models of stellar pulsations. Surface layers, rotation, and magnetic fields imprint erratic frequency…

Solar and Stellar Astrophysics · Physics 2015-06-04 M. Gruberbauer , D. B. Guenther , T. Kallinger

Asteroseismology is an exceptional tool for studying stars by using the properties of observed modes of oscillation. So far the process of performing an asteroseismic analysis of a star has remained somewhat esoteric and inaccessible to…

This review outlines concepts of mathematical statistics, elements of probability theory, hypothesis tests and point estimation for use in the analysis of modern astronomical data. Least squares, maximum likelihood, and Bayesian approaches…

Instrumentation and Methods for Astrophysics · Physics 2012-05-10 Eric D. Feigelson , G. Jogesh Babu

Almost 100 years ago Sir Arthur Eddington noted that the interiors of stars were inaccessible to observations. The advent of helio- and asteroseismology has completely changed this assessment. Helioseismology has provided very detailed…

Solar and Stellar Astrophysics · Physics 2016-02-23 J. Christensen-Dalsgaard

The interpretation of pulsation data for Sun-like stars is currently facing challenges quite similar to those faced by white dwarf modelers ten years ago. The observational requirements for uninterrupted long-term monitoring are beginning…

Astrophysics · Physics 2009-11-10 Travis S. Metcalfe

We present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5d of science operations, reveal high signal-to-noise solar-like oscillation spectra in all…

Solar and Stellar Astrophysics · Physics 2015-05-14 W. J. Chaplin , T. Appourchaux , Y. Elsworth , R. A. Garcia , G. Houdek , C. Karoff , T. S. Metcalfe , J. Molenda-Zakowicz , M. J. P. F. G. Monteiro , M. J. Thompson , T. M. Brown , J. Christensen-Dalsgaard , R. L. Gilliland , H. Kjeldsen , W. J. Borucki , D. Koch , J. M. Jenkins , J. Ballot , S. Basu , M. Bazot , T. R. Bedding , O. Benomar , A. Bonanno , I. M. Brandao , H. Bruntt , T. L. Campante , O. L. Creevey , M. P. Di Mauro , G. Dogan , S. Dreizler , P. Eggenberger , L. Esch , S. T. Fletcher , S. Frandsen , N. Gai , P. Gaulme , R. Handberg , S. Hekker , R. Howe , D. Huber , S. G. Korzennik , J. C. Lebrun , S. Leccia , M. Martic , S. Mathur , B. Mosser , R. New , P. -O. Quirion , C. Regulo , I. W. Roxburgh , D. Salabert , J. Schou , S. G. Sousa , D. Stello , G. A. Verner , T. Arentoft , C. Barban , K. Belkacem , S. Benatti , K. Biazzo , P. Boumier , P. A. Bradley , A. -M. Broomhall , D. L. Buzasi , R. U. Claudi , M. S. Cunha , F. D'Antona , S. Deheuvels , A. Derekas , A. Garcia Hernandez , M. S. Giampapa , M. J. Goupil , M. Gruberbauer , J. A. Guzik , S. J. Hale , M. J. Ireland , L. L. Kiss , I. N. Kitiashvili , K. Kolenberg , H. Korhonen , A. G. Kosovichev , F. Kupka , Y. Lebreton , B. Leroy , H. -G. Ludwig , S. Mathis , E. Michel , A. Miglio , J. Montalban , A. Moya , A. Noels , R. W. Noyes , P. L. Palle , L. Piau , H. L. Preston , T. Roca Cortes , M. Roth , K. H. Sato , J. Schmitt , A. M. Serenelli , V. Silva Aguirre , I. R. Stevens , J. C. Suarez , M. D. Suran , R. Trampedach , S. Turck-Chieze , K. Uytterhoeven , R. Ventura

Asteroseismology, the study of stellar oscillations, provides high-precision measurements of masses and ages for red giants. Scaling relations are a powerful tool for measuring fundamental stellar parameters, and the derived radii are in…

Solar and Stellar Astrophysics · Physics 2025-12-09 Kaili Cao , Marc H. Pinsonneault

Asteroseismology of solar-type stars has entered a new era of large surveys with the success of the NASA \textit{Kepler} mission, which is providing exquisite data on oscillations of stars across the Hertzprung-Russell (HR) diagram. From…

Oscillation frequencies are the most accurate properties one can measure for a star, potentially allowing detailed tests of stellar models and evolution theories. We briefly review asteroseismology for two classes of stars. In delta Scuti…

Astrophysics · Physics 2007-05-23 Hans Kjeldsen , Timothy R. Bedding

We give here the Table of Contents and clickable links to papers of the proceedings from the workshop "Asteroseismology of Stellar Populations in the Milky Way", held in Sesto, 22-26 July 2013. The aim of this workshop was to foster…

Solar and Stellar Astrophysics · Physics 2015-06-22 Andrea Miglio , Patrick Eggenberger , Leo Girardi , Josefina Montalban

Eddington, COROT, MONS, KEPLER, and the other asteroseismology and planet finding missions, obtain extremely high photometric quality time-series data as their primary purpose. Similar quality data are potentially, and in some designs…

Astrophysics · Physics 2007-05-23 G. Gilmore
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