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Numerical Hydrodynamics and Magnetohydrodynamics in General Relativity. [PDF]
Font JA.
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Physics of Neutron Star Crusts. [PDF]
Chamel N, Haensel P.
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Astrospheres and Solar-like Stellar Winds. [PDF]
Wood BE.
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Annual Review of Astronomy and Astrophysics, 1994
Carl J. Hansen, Steven D. Kawaler
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Carl J. Hansen, Steven D. Kawaler
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2013
Our understanding of stars has grown significantly due to recent advances in asteroseismology, the stellar analog of helioseismology, the study of the Sun's acoustic wave oscillations. Using ground-based and satellite observatories to measure the frequency spectra of starlight, researchers are able to probe beneath a star's surface and map its interior
openaire +1 more source
Our understanding of stars has grown significantly due to recent advances in asteroseismology, the stellar analog of helioseismology, the study of the Sun's acoustic wave oscillations. Using ground-based and satellite observatories to measure the frequency spectra of starlight, researchers are able to probe beneath a star's surface and map its interior
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Asteroseismology: results and prospects
Symposium - International Astronomical Union, 1988Asteroseismology is interpreted as an extension of the field of variable stars, and not just as the stellar analogue of helioseismology. The main effects of stellar mass and evolution on oscillation frequencies are discussed with the help of simplified wave-propagation diagrams.
W. Däppen +2 more
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Gravitational wave asteroseismology reexamined
Physical Review D, 2004The frequencies and damping times of the non radial oscillations of non rotating neutron stars are computed for a set of recently proposed equations of state (EOS) which describe matter at supranuclear densities. These EOS are obtained within two different approaches, the nonrelativistic nuclear many-body theory and the relativistic mean field theory ...
O. BENHAR +2 more
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Asteroseismology and interferometry .
2006International ...
Thévenin, Frédéric +5 more
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