Results 21 to 30 of about 22,085 (227)
Universe, 2021 Lead (Pb) is predicted to have large over-abundances with respect to other s-process elements in Asymptotic Giant Branch (AGB) stars, especially of low metallicities.
Devika Kamath, Hans Van Winckel
doaj +1 more source
Pulsation-triggered dust production by asymptotic giant branch stars [PDF]
Monthly notices of the Royal Astronomical Society, 2018 Eleven nearby (
I. McDonald +3 more
semanticscholar +1 more source
Heavy-element yields and abundances of asymptotic giant branch models with a Small Magellanic Cloud metallicity [PDF]
, 2018 We present new theoretical stellar yields and surface abundances for asymptotic giant branch (AGB) models with a metallicity appropriate for stars in the Small Magellanic Cloud (SMC, $Z= 0.0028$, [Fe/H] $\approx -0.7$).
Amanda I Karakas +5 more
semanticscholar +1 more source
Magnetic and non-magnetic AGB mixing for s-processing [PDF]
EPJ Web of Conferences, 2023 I outline a few features of recent models for the formation of the neutron source 13C(α,n)16O in low mass stars (1 ≲ M/M⊙ ≲ 3, LMS ) ascendingfor the second time the Red Giant Branch, generally called Asymptotic Giant Branch, or AGB stars. I also briefly
Busso Maurizio
doaj +1 more source
STELLAR YIELDS FROM METAL-RICH ASYMPTOTIC GIANT BRANCH MODELS [PDF]
, 2016 We present new theoretical stellar yields and surface abundances for three grids of metal-rich asymptotic giant branch (AGB) models. Post-processing nucleosynthesis results are presented for stellar models with initial masses between 1 M☉ and 7.5 M☉ for ...
A. Karakas, M. Lugaro
semanticscholar +1 more source
Infrared Properties of Asymptotic Giant Branch Stars in Our Galaxy and the Magellanic Clouds [PDF]
Astrophysical Journal, 2019 We investigate the infrared properties of asymptotic giant branch (AGB) stars in our Galaxy and the Magellanic Clouds using various infrared observational data and theoretical models.
K. Suh
semanticscholar +1 more source
ASYMPTOTIC GIANT BRANCH VARIABLES
Odessa Astronomical Publications, 2017 Asymptotic Giant Branch variable are the brightest and most distinctive individual stars to be found in the resolved, old and inter mediate age, stellar populations of galaxies in the Local Group and beyond.
P. A. Whitelock
doaj +1 more source
The Search for Binaries in Post-Asymptotic Giant Branch Stars: Do Binary Companions Shape the Nebulae? [PDF]
Journal of Astronomy and Space Sciences, 2012 Binary companions are often invoked to explain the axial and point symmetry seen in the majority of planetary nebulae and proto-planetary nebulae (PPNs).
Bruce J. Hrivnak
doaj +1 more source
Studying Asymptotic Giant Branch Stars in the JWST Era
Universe, 2020 We explore the potential offered by the incoming launch of the James Webb Space Telescope, to study the stars evolving through the asymptotic giant branch (AGB) phase. To this aim we compare data of AGB stars in the Large Magellanic Cloud, taken with the
Paolo Ventura +3 more
doaj +1 more source
Rotation of the asymptotic giant branch star R Doradus [PDF]
, 2018 High resolution observations of the extended atmospheres of asymptotic giant branch (AGB) stars can now directly confront the theories that describe stellar mass loss. Using Atacama Large Millimeter/submillimeter Array (ALMA) high angular resolution ($30\
W. Vlemmings +9 more
semanticscholar +1 more source