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Nuclear Neutrino Spectra in Late Stellar Evolution [PDF]
EPJ Web of Conferences, 2018 Neutrinos are the principle carriers of energy in massive stars, beginning from core carbon burning and continuing through core collapse and after the core bounce. In fact, it may be possible to detect neutrinos from nearby pre-supernova stars. Therefore,
Misch G. Wendell +2 more
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UniverseThe rapid growth of large-scale astronomical surveys and advances in data-driven analysis techniques have transformed the study of late-stage stellar evolution.
Princy Ranaivomanana, Murat Uzundag
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Perspectives on the physics of late-type stars from beyond low earth orbit, the moon and mars [PDF]
npj MicrogravityWith the new discoveries enabled thanks to the recent space missions, stellar physics is going through a revolution. However, these discoveries opened the door to many new questions that require more observations.
Savita Mathur, Ângela R. G. Santos
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Late Stages of Stellar Evolution [PDF]
Astrophysics and Space Science Library, 1987 exaly +2 more sources
Screening Factors in Late Stellar Evolution [PDF]
Symposium - International Astronomical Union, 1974 Recent studies (DeWitt et al., 1973; Graboske et al., 1973) have modified the screening factors for nuclear reactions. The theory develops a general statistical mechanical framework within which the various analytical models of Salpeter are combined with Monte Carlo and perturbation calculations for specific mixtures.
Harold C. Graboske, Hugh E. DeWitt
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The Astrophysical Journal, 2023 The ages of solar-like stars have been at the center of many studies such as exoplanet characterization or Galactic-archeology. While ages are usually computed from stellar evolution models, relations linking ages to other stellar properties, such as ...
Savita Mathur +11 more
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Late stages of stellar evolution with PLANCK [PDF]
Proceedings of CMB and Physics of the Early Universe — PoS(CMB2006), 2007 The Planck mission may, in principle, have a large impact on stellar studies because it will cover a very important observational band. For various classes of stellar objects continuum observations at millimetric and submillimetric wavelengths would be very fruitful, because they provide essential clues to understand the physics of these stars and ...
Grazia Umana +4 more
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X-ray Observations of Planetary Nebulae since WORKPLANS I and Beyond
Galaxies, 2020 Planetary nebulae (PNe) were expected to be filled with hot pressurized gas driving their expansion. ROSAT hinted at the presence of diffuse X-ray emission from these hot bubbles and detected the first sources of hard X-ray emission from their central ...
Martín A. Guerrero
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Planetary Engulfment Prognosis within the ρ CrB System
The Astrophysical Journal, 2023 Exoplanets have been detected around stars at various stages of their lives, ranging from young stars emerging from formation to the latter stages of evolution, including white dwarfs and neutron stars.
Stephen R. Kane
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