Inefficient Growth of SiOx Grains : Implications for Circumstellar Outflows
To explain observations of abundant circumstellar dust and high stellar wind velocity, most models simply postulate the efficient nucleation and growth of silicate dust particles. Here, we report measurement of the SiO-(SiOx)(n) grain sticking coefficient in a microgravity sounding rocket experiment, indicating very inefficient (0.005-0.016) grain ...
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Abundant supernova dust and heterogeneous aqueous alteration revealed by stardust in two lithologies of asteroid Bennu. [PDF]
Nguyen AN +10 more
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Formation of SiC grains in circumstellar envelops of carbon stars
The emission feature around 11.3 micrometer observed towards carbon stars is considered to be due to SiC grains condensed in the circumstellar envelopes. The isotopic anomalies of SiC discovered in carbonaceous meteorites strongly support the formation of SiC grains in carbon-rich AGB (Asymptotic Giant Branch) stars.
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Computational investigation of spin-resolved energy landscapes of FeC<sub>4</sub>H<sub>2</sub> <sup>+</sup> and their astrochemical implications. [PDF]
Shajan S, Thirumoorthy K.
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Direct Samples of Interstellar and Interplanetary Material with IMAP. [PDF]
Szalay JR +21 more
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Some Possible Components of Circumstellar Grain Material
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The chemistry of habitable oceans in the Solar system. [PDF]
Hao J +17 more
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Modeling the radiolysis in H<sub>2</sub>O : HCOOH ice: connecting laboratory experiments with astronomical measurements. [PDF]
Fargnoli CMF, Moraes L, Pilling S.
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Chemistry in Extreme Environments: The Mystery of Molecular Complexity in Space. [PDF]
Puzzarini C, Alessandrini S.
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Origin and Evolution of the Galilean Satellites Within the Jovian System. [PDF]
Nimmo F +10 more
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