The physics and chemistry of circumstellar envelopes of S-stars on the AGB
Presented here are the preliminary results of a long-term study of S-stars on the AGB. S-stars are important as possible transition objects between oxygen-rich M-stars and carbon stars.
Olofsson, Hans, +2 more
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An axisymmetric shock breakout indicated by prompt polarized emission from the type II supernova 2024ggi. [PDF]
Yang Y +20 more
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Experimental evidence for granular shear-flow instability in the Epstein regime. [PDF]
Capelo HL +9 more
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n-Alkanes formed by methyl-methylene addition as a source of meteoritic aliphatics. [PDF]
Merino P +16 more
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Spiers Memorial Lecture: Astrochemistry at high resolution.
Ceccarelli C.
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Silicon and Hydrogen Chemistry under Laboratory Conditions Mimicking the Atmosphere of Evolved Stars. [PDF]
Accolla M +12 more
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Swift Heavy Ion-Induced Chemistry of CH<sub>3</sub>CN Ices at 10 and 80 K. [PDF]
de Barros ALF +10 more
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A probable Keplerian disk feeding an optically revealed massive young star. [PDF]
McLeod AF +5 more
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Direct Samples of Interstellar and Interplanetary Material with IMAP. [PDF]
Szalay JR +21 more
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Supernovae and transients with circumstellar interaction. [PDF]
Fraser M.
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