Results 141 to 150 of about 3,760 (219)

Acoustic modes in M67 cluster stars trace deepening convective envelopes. [PDF]

open access: yesNature
Reyes C   +5 more
europepmc   +1 more source

The <sup>22</sup>Ne( α ,n)<sup>25</sup>Mg reaction - state of the art, astrophysics, and perspectives. [PDF]

open access: yesEur Phys J A Hadron Nucl
Best A   +13 more
europepmc   +1 more source

Common envelope binary interaction simulations between a thermally pulsating AGB star and a low mass companion. [PDF]

open access: yesMon Not R Astron Soc, 2022
González-Bolívar M   +4 more
europepmc   +1 more source

History of individual presolar SiC grains revealed by stellar winds. [PDF]

open access: yesNat Commun
Bajo KI   +4 more
europepmc   +1 more source

Carbonaceous dust grains seen in the first billion years of cosmic time. [PDF]

open access: yesNature, 2023
Witstok J   +41 more
europepmc   +1 more source

Pulsation Properties in Asymptotic Giant Branch Stars

open access: yes, 2019
Asymptotic Giant Branch (AGB) stars are stars with low- to intermediate mass in a late stage in their stellar evolution. An important feature of stellar evolution is the ongoing nucleosynthesis, the creation of heavier elements.
Norgren, Ofelia
core  

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