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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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Asteroseismology and Dynamics Reveal Interior Structure and Coeval Evolution in the Triply Post-Main-Sequence system DG Leo [PDF]
Ping Li +6 more
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Relativistic Fluid Dynamics: Physics for Many Different Scales. [PDF]
Andersson N, Comer GL.
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Asteroseismology of Triple-mode Radial δ Scuti Star: TIC 400562821
Xiaoya Sun +5 more
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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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