Results 91 to 100 of about 4,442 (177)

Population Synthesis Models including AGB Stars and their Ingredients

open access: yes, 2007
I briefly review the state of the art of evolutionary population synthesis (EPS) models that include the contribution from AGB ...
MARIGO, PAOLA
core  

Headwind: Modelling Mass Loss of AGB Stars, Against All Odds

open access: yes, 2007
The intricate interplay of atmospheric shock waves and a complex, variable radiation field with non-equilibrium dust formation presents a considerable challenge to self-consistent modelling of atmospheres and winds of AGB stars.
Höfner, Susanne,
core  

Binaries in AGB and post-AGB stars at high resolution

open access: yes, 2019
Binary stellar systems are very interesting cosmic laboratories, as they are related to many astrophysical phenomena, from the genesis of SNIa in post common envelope systems, to gravitational waves. They are also the most likely explanation of the formation of non-spherical axisymmetric PNe, a long standing problem in the field of late stellar ...
openaire   +2 more sources

Exploring the extended atmospheres of AGB stars [Elektronisk resurs]

open access: yes
Stars evolve along various paths depending primarily on their initial masses, undergoing changes in internal structure and processes that affect their temperature, size, and surface abundances.
Bojnordiarbab, Behzad,
core  

Interferometric studies of AGB and post-AGB stars

open access: yes, 2013
Several classes of evolved stars contain highly luminous objects, which, more often than not, are characterized by strong mass loss. Two fundamental properties that lie at the basis of their outer appearance and internal evolution, as well as that of the galaxies in which they are embedded.
openaire   +1 more source

The abundance of S- and Si-bearing molecules in O-rich circumstellar envelopes of AGB stars. [PDF]

open access: yesAstron Astrophys, 2020
Massalkhi S   +3 more
europepmc   +1 more source

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