Results 211 to 220 of about 6,468 (258)
Physics of Neutron Star Crusts. [PDF]
Living Rev Relativ, 2008 Chamel N, Haensel P.
europepmc +1 more source
Astrospheres and Solar-like Stellar Winds. [PDF]
Living Rev Sol Phys, 2004 Wood BE.
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Constraining equation-of-state groups from g-mode asteroseismology [PDF]
Monthly Notices of the Royal Astronomical Society, 2022 Buoyancy-restored modes inside neutron stars depend sensitively on both the microphysical (e.g., composition and entropy gradients) and macrophysical (e.g., stellar mass and radius) properties of the star.
Hao-Jui Kuan +2 more
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Integrated mass-loss of evolved stars in M4 using asteroseismology [PDF]
Monthly Notices of the Royal Astronomical Society, 2022 Mass loss remains a major uncertainty in stellar modelling. In low-mass stars, mass loss is most significant on the red giant branch (RGB), and will impact the star’s evolutionary path and final stellar remnant.
Madeline Howell +2 more
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A calibration of the Rossby number from asteroseismology [PDF]
Astronomy and Astrophysics, 2021 Stellar activity and rotation are tightly related in a dynamo process. Our understanding of this mechanism is mainly limited by our capability of inferring the properties of stellar turbulent convection.
E Corsaro, A Bonanno, S Mathur
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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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Asteroseismology and interferometry .
2006International ...
Thévenin, Frédéric +5 more
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