Can Isotopologues Be Used as Biosignature Gases in Exoplanet Atmospheres? [PDF]
Glidden A +3 more
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Acoustic modes in M67 cluster stars trace deepening convective envelopes. [PDF]
Reyes C +5 more
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The <sup>22</sup>Ne( α ,n)<sup>25</sup>Mg reaction - state of the art, astrophysics, and perspectives. [PDF]
Best A +13 more
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Common envelope binary interaction simulations between a thermally pulsating AGB star and a low mass companion. [PDF]
González-Bolívar M +4 more
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History of individual presolar SiC grains revealed by stellar winds. [PDF]
Bajo KI +4 more
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Carbonaceous dust grains seen in the first billion years of cosmic time. [PDF]
Witstok J +41 more
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Exploring central star variability of planetary nebulae using gaia photometry. [PDF]
NegmEldin MA, Ali A, Hamid GM, Essam A.
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Pulsation Properties in Asymptotic Giant Branch Stars
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
Perspectives on the physics of late-type stars from beyond low earth orbit, the moon and mars. [PDF]
Mathur S, Santos ÂRG.
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The Formation of MgS & MgO Monomers and Dimers from Magnesium, Oxygen, and Sulfur Hydrides. [PDF]
Bell KM, Fortenberry RC.
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