Results 11 to 20 of about 214,013 (271)
Effects of thermohaline instability and rotation-induced mixing on the evolution of light elements in the Galaxy : D, 3He and 4He [PDF]
Recent studies of low- and intermediate-mass stars show that the evolution of the chemical elements in these stars is very different from that proposed by standard stellar models.
Asplund+88 more
core +2 more sources
Rotation and Stellar Evolution [PDF]
Does rotation influence stellar evolution? Does it cause observational effects other than line broadening? Can rotation be responsible for mixing of chemical elements throughout the star? Do evolved stars have rapidly rotating cores? This, for instance, is of interest if one wants to compute the details of supernova events.
H.-C. Thomas, R. Kippenhahn
openaire +1 more source
Linking the formation and fate of exo-Kuiper belts within solar system analogues [PDF]
Escalating observations of exo-minor planets and their destroyed remnants both passing through the solar system and within white dwarf planetary systems motivate an understanding of the orbital history and fate of exo-Kuiper belts and planetesimal discs.
Cai, Maxwell X.+9 more
core +3 more sources
On the parallelization of stellar evolution codes [PDF]
AbstractMultidimensional nucleosynthesis studies with hundreds of nuclei linked through thousands of nuclear processes are still computationally prohibitive. To date, most nucleosynthesis studies rely either on hydrostatic/hydrodynamic simulations in spherical symmetry, or on post-processing simulations using temperature and density versus time ...
Martin Rodriguez, David+2 more
openaire +5 more sources
Trends of stellar entropy along stellar evolution [PDF]
17 pages, 3 figures, accepted for publication at Research in Astronomy and Astrophysics (RAA)
Jorge Ernesto Horvath+2 more
openaire +3 more sources
The evolution of stellar exponential discs [PDF]
12 pages inclding 9 figures, MNRAS ...
Annette M. N. Ferguson, Catherine Clarke
openaire +5 more sources
The stellar masses, mean ages, metallicities, and star formation histories of galaxies are now commonly estimated via stellar population synthesis (SPS) techniques.
Abazajian+80 more
core +1 more source
The Geneva stellar evolution code [PDF]
This paper presents the Geneva stellar evolution code with special emphasis on the modeling of solar-type stars. The basic input physics used in the Geneva code as well as the modeling of atomic diffusion is first discussed. The physical description of rotation is then presented.
Suzanne Talon+7 more
openaire +4 more sources