Results 51 to 60 of about 10,149 (153)
Asteroseismology of the GW Virginis stars SDSS J0349-0059 and VV 47 [PDF]
We present an asteroseismological study of SDSS J0349-0059 and VV 47 aimed mainly at deriving their total mass on the basis of state-of-the-art PG 1159 evolutionary models.
Althaus, Leandro G. +2 more
core +3 more sources
Current issues in asteroseismology
In this contribution we briefly review some of the current issues and promises for the future by asteroseismology. We are entering a new phase in this field driven by the wealth of data that has been collected and data that will soon be available for asteroseismology across the HR Diagram.
Bazot, Michael +2 more
openaire +2 more sources
We report an analysis of the first known Beta Cep pulsator observed by the TESS mission, the runaway star PHL 346 = HN Aqr. The star, previously known as a singly-periodic pulsator, has at least 34 oscillation modes excited, 12 of those in the g-mode ...
Aliçavuş, Filiz Kahraman +23 more
core +1 more source
We aim at studying the theoretical properties of the regular spacings found in the oscillation spectra of delta Scuti stars. We performed a multi-variable analysis covering a wide range of stellar structure and seismic properties and model parameters ...
A. García Hernández +62 more
core +1 more source
In this article, we show how asteroseismology and spectropolarimetry allow to probe dynamical processes in massive star interiors. First, we give a summary of the state-of-the-art.
Mathis, Stéphane, Neiner, Coralie
core +1 more source
Measurements of Stellar Properties through Asteroseismology: A Tool for Planet Transit Studies
Oscillations occur in stars of most masses and essentially all stages of evolution. Asteroseismology is the study of the frequencies and other properties of stellar oscillations, from which we can extract fundamental parameters such as density, mass ...
Bedding +7 more
core +1 more source
An asteroseismology explorer [PDF]
In response to a NASA opportunity, a proposal has been made to study the concept of an Asteroseismology Explorer (ASE). The goal of the ASE would be to measure solar-like oscillations on many (perhaps hundreds) of stars during a 1-year mission, including many members of open clusters.
Brown, T. M., Cox, A. N.
openaire +1 more source
21 pages; This is a pre-print of an invited chapter for the Encyclopedia of Astrophysics (edited by I. Mandel, section editor F.R.N.
Bowman, Dominic M., Bugnet, Lisa
openaire +2 more sources
We present results of a long-baseline interferometry campaign using the PAVO beam combiner at the CHARA Array to measure the angular sizes of five main-sequence stars, one subgiant and four red giant stars for which solar-like oscillations have been ...
Aguirre, V. Silva +39 more
core +1 more source
The imprint of star formation on stellar pulsations. [PDF]
Steindl T, Zwintz K, Vorobyov E.
europepmc +1 more source

