Results 11 to 20 of about 3,339,915 (332)
EPJ Web of Conferences, 2023 Polytropes, Virial theorem, evolutionary time scales, degrees of freedom, radiative transport, molecular weight, degeneracy, Jeans mass, and Eddington luminosity are basic ingredients to describe the physics of stars.
Palmerini S.
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Population Synthesis to Constrain Galactic and Stellar Physics - I. Determining Age and Mass of Thin-Disc Red-Giant Stars [PDF]
Astronomy and Astrophysics, 2017 Context. The cornerstone mission of the European Space Agency, Gaia , together with forthcoming complementary surveys (CoRoT, Kepler , K2, APOGEE, and Gaia -ESO), will revolutionize our understanding of the formation and history of our Galaxy, providing ...
Annie Robin +2 more
exaly +2 more sources
Living Reviews in Solar PhysicsMagnetic storms on stars manifest as remarkable, randomly occurring changes of the luminosity over durations that are tiny in comparison to the normal evolution of stars.
Adam F. Kowalski
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Chemical element transport in stellar evolution models [PDF]
Royal Society Open Science, 2017 Stellar evolution computations provide the foundation of several methods applied to study the evolutionary properties of stars and stellar populations, both Galactic and extragalactic.
Maurizio Salaris, Santi Cassisi
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Blue supergiants as tests for stellar physics [PDF]
Astronomy & Astrophysics, 2021 Context. Massive star evolution is still poorly understood, and observational tests are required to discriminate between different implementations of physical phenomena in stellar evolution codes. Aims.
C. Georgy, H. Saio, G. Meynet
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Multiband gravitational-wave event rates and stellar physics [PDF]
Physical Review D, 2019 Joint gravitational-wave detections of stellar-mass black-hole binaries by ground- and space-based observatories will provide unprecedented opportunities for fundamental physics and astronomy.
D. Gerosa +6 more
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Evidence for spots on hot stars suggests major revision of stellar physics [PDF]
Monthly notices of the Royal Astronomical Society, 2019 It has long been thought that starspots are not present in the A and B stars because magnetic fields cannot be generated in stars with radiative envelopes. Space observations show that a considerable fraction of these stars varies in light with periods
L. Balona
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Journal of Astronomical Telescopes Instruments and Systems, 2022 . The Extreme-ultraviolet Stellar Characterization for Atmospheric Physics and Evolution (ESCAPE) mission is an astrophysics Small Explorer employing ultraviolet spectroscopy (EUV: 80 to 825 Å and FUV: 1280 to 1650 Å) to explore the high-energy radiation
K. France +29 more
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Role of stellar physics in regulating the critical steps for life [PDF]
International Journal of Astrobiology, 2018 We use the critical step model to study the major transitions in evolution on Earth. We find that a total of five steps represents the most plausible estimate, in agreement with previous studies, and use the fossil record to identify the potential ...
M. Lingam, A. Loeb
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