Results 51 to 60 of about 985,930 (333)
Modules for Experiments in Stellar Astrophysics ( ): Convective Boundaries, Element Diffusion, and Massive Star Explosions [PDF]
, 2017 We update the capabilities of the software instrument Modules for Experiments in Stellar Astrophysics (MESA) and enhance its ease of use and availability.
B. Paxton +17 more
semanticscholar +1 more source
The Astrophysical Journal, 2023 The Hubble Space Telescope (HST)/Space Telescope Imaging Spectrograph treasury program Advanced Spectral Library enables investigations of the characteristics and dynamics of the wind and chromosphere of cool stars using high-quality spectral data.
Krister E. Nielsen +3 more
doaj +1 more source
Physics of Rotation in Stellar Models [PDF]
, 2009 32 pages, 7 figures, lectures, CNRS school, will be published by ...
openaire +3 more sources
parsec: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code [PDF]
, 2012 We present the updated version of the code used to compute stellar evolutionary tracks in Padova. It is the result of a thorough revision of the major in put physics, together with the inclusion of the pre‐main sequence phase, not present in our previous
A. Bressan +6 more
semanticscholar +1 more source
First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies [PDF]
, 2017 The IllustrisTNG project is a new suite of cosmological magneto-hydrodynamical simulations of galaxy formation performed with the Arepo code and updated models for feedback physics.
A. Pillepich +10 more
semanticscholar +1 more source
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
doaj +1 more source
Approximate input physics for stellar modelling [PDF]
Monthly Notices of the Royal Astronomical Society, 1995 We present a simple and efficient, yet reasonably accurate, equation of state, which at the moderately low temperatures and high densities found in the interiors of stars less massive than the Sun is substantially more accurate than its predecessor by Eggleton, Faulkner & Flannery.
Zhanwen Han +3 more
openaire +3 more sources
The origin and evolution of the odd-Z iron-peak elements Sc, V, Mn, and Co in the Milky Way stellar disk ?,?? [PDF]
, 2015 AIMS: The aim of this study is to investigate the origin and evolution of Sc, V, Mn, and Co for a homogeneous and statistically significant sample of stars probing the different populations of the Milky Way, in particular the thin and thick disks ...
C. Battistini +5 more
semanticscholar +1 more source
Fifty Years After the Discovery of the First Stellar-Mass Black Hole: A Review of Cyg X-1
GalaxiesAround 50 years ago, the famous bet between Stephen Hawking and Kip Thorne on whether Cyg X-1 hosts a stellar-mass black hole became a well-known story in the history of black hole science.
Jiachen Jiang
doaj +1 more source
EPJ Web of Conferences, 2017 The unparalleled photometric data obtained by NASA’s Kepler Space Telescope has led to an improved understanding of stellar structure and evolution - in particular for solar-like oscillators in this context. Binary stars are fascinating objects.
Beck P. G. +12 more
doaj +1 more source