Results 21 to 30 of about 4,355,728 (290)
Habitable Environments in Late Stellar Evolution
, 2021 With very high potential transit-depths and no stellar flare activity, the planets of White Dwarfs are some of the most promising in the search for detectable extraterrestrial life. We review the evidence that both terrestrial and gas-giant planets are capable of surviving post-main sequence evolution and migrating into the WD phase.
Dewy Peters +1 more
openaire +2 more sources
Solar-Like Oscillators in the Kepler Era: A Review
Frontiers in Astronomy and Space Sciences, 2021 Many late-type stars across the Milky Way exhibit observable pulsations similar to our Sun that open up a window into stellar interiors. The NASA Kepler mission, a space-based photometric telescope, measured the micro-magnitude luminosity fluctuations ...
Jason Jackiewicz
doaj +1 more source
STEllAR-GROUP/octotiger: Kokkos kernels
, 2021 What's Changed Branch by @diehlpk in https://github.com/STEllAR-GROUP/octotiger/pull/341 Add Zenodo DOI by @diehlpk in https://github.com/STEllAR-GROUP/octotiger/pull/342 Docu by @diehlpk in https://github.com/STEllAR-GROUP/octotiger/pull/347 Add ...
Biddiscombe, John +10 more
core +1 more source
Late stages of stellar evolution – Herschel’s contributions [PDF]
Advances in Space Research, 2012 Cool objects glow in the infrared. The gas and solid-state species that escape the stellar gravitational attraction of evolved late-type stars in the form of a stellar wind are cool, with temperatures typically $\la$1500\,K, and can be ideally studied in the infrared.
openaire +2 more sources
Seismic Cartography of White-Dwarf Interiors From the Toulouse-Montréal Optimal-Design Approach
Frontiers in Astronomy and Space Sciences, 2022 Probing internal properties of white-dwarf stars has been amongst the earliest objectives of asteroseismology, following the first discovery in the late 1960s of non-radial pulsations in these evolved compact stars.
Noemi Giammichele +2 more
doaj +1 more source
M-dwarf stellar winds : the effects of realistic magnetic geometry on rotational evolution and planets [PDF]
, 2014 AAV acknowledges support from a Royal Astronomical Society Fellowship. JM acknowledges support from a fellowship of the Alexander von Humboldt foundation.We perform three-dimensional numerical simulations of stellar winds of early-M-dwarf stars.
Morin, J. +12 more
core +1 more source
Late-time behavior of stellar collapse and explosions. II. Nonlinear evolution [PDF]
Physical Review D, 1994 23pp, RevTex, 15 figures (included), NSF-ITP-93 ...
, Gundlach, , Price, , Pullin
openaire +3 more sources
What drives stellar population evolution?
, 2019 The stellar population of a galaxy contains a record of its star formation and assembly history, making it an important area of research to develop our understanding of galaxy formation and evolution.
Barone, Tania (6908315)
core +1 more source
A review of the search for AGB stars
Frontiers in Astronomy and Space SciencesThe Asymptotic Giant Branch (AGB) is the late stage of the evolution of intermediate and low-mass stars and is of great importance for understanding stellar evolution, nucleosynthesis, and the chemical evolution of galaxies.
Hai-Ling Lu +15 more
doaj +1 more source
Pediatric Blood &Cancer, EarlyView.ABSTRACT Background Loneliness is associated with adverse physical and mental health outcomes and remains understudied in children and adolescents undergoing cancer therapy. Pediatric oncology patients may be at increased risk due to medical isolation and disruption of social networks.
Charlotte N. Stahlfeld +5 more
wiley +1 more source