Results 1 to 10 of about 1,846,404 (321)
Mass Loss and Supernova Progenitors [PDF]
7 pages, 3 figures, to appear in the Conference Proceedings of "Unsolved Problems in Stellar Astrophysics"
John Eldridge +4 more
openaire +3 more sources
Advances in mass-loss predictions [PDF]
Universidad de ...
Vink, J.S. +4 more
openaire +7 more sources
Crystallinity versus mass-loss rate in asymptotic giant branch stars [PDF]
Infrared Space Observatory (ISO) observations have shown that O-rich Asymptotic Giant Branch (AGB) stars exhibit crystalline silicate features in their spectra only if their mass-loss rate is higher than a certain threshold value.
F. Kemper +3 more
openalex +6 more sources
Red Supergiant Mass Loss and Mass-Loss Rates
This review discusses the causes, nature, importance and observational evidence of mass loss by red supergiants. It arrives at the perception that mass loss finds its origin in the gravity which makes the star a star in the first place, and is a ...
Jacco Th. van Loon
doaj +3 more sources
Observational evidence for mass loss from cool stars is reviewed. Spectra line profiles are used for the derivation of mass-loss rates with the aid of the equation of continuity. This equation implies steady mass loss with spherical symmetry.
Goldberg, Leo
openaire +3 more sources
MBD analysis of flexible multibody system with mass loss
In this paper, we propose a formulation method for flexible multi-body systems with mass loss. The method derives the equation of motion using the velocity transformation method, in consideration of the shift of center-of-mass.
Kanjuro MAKIHARA +2 more
doaj +3 more sources
Orbital Migration Through Atmospheric Mass Loss
Atmospheric mass loss is thought to have strongly shaped the sample of close-in exoplanets. These atmospheres should be lost isotropically, leading to no net migration on the planetary orbit.
Benjamin Hanf +4 more
doaj +3 more sources
Phenotypic plasticity in mass loss during chick rearing in the European starling (Sturnus vulgaris) [PDF]
It has long been recognized that mass loss during breeding could be adaptive (e.g., by ameliorating the costs of increased parental activity). However, many studies still commonly interpret mass loss as evidence of “stress” or a cost of reproduction (i.e.
Brett L. Hodinka, Tony D. Williams
doaj +2 more sources
Modeling of the Wind/Disk Outflow from Be Stars II: Formation of the Keplerian Disk
Computer modeling of the outflow from Be stars is performed. In our approach, processes of turbulence excitation and turbulent viscosity are added to the conventional model of the radiation driven winds.
Sergey Bogovalov, Maxim Petrov
doaj +1 more source
Modeling of the Wind/Disk Outflow from Be Stars
The objective of this work is to reproduce the formation of the fast polar wind and viscous disk outflow from Be stars in a unified physical picture. Numerical modeling of the plasma outflow from fast rotating stars was performed taking into account the ...
Sergey Bogovalov, Maxim Petrov
doaj +1 more source

