We report on the isotopic, chemical, and structural properties of four O-rich presolar grains identified in situ in the Adelaide ungrouped C2, LaPaZ Icefield (LAP) 031117 CO3.0, and Dominion Range (DOM) 08006 CO3.0 chondrites. All four grains have oxygen-isotopic compositions consistent with origins in the circumstellar envelopes (CSE) of low-mass O-rich stars evolved along the red-giant and asymptotic-giant branch (RGB, AGB, respectively) of stellar evolution. Transmission electron microscope (TEM) analyses, enabled by focused-ion-beam scanning electron microscope extraction, show that the grain from Adelaide is a single-crystal Mg-Al spinel, and comparison with equilibrium thermodynamic predictions constrains its condensation to 1500 K as...
Presolar oxide grains have been previously divided into several groups (Group 1 to 4) based on their...
International audienceCI chondrites have nonvolatile chemical compositions closely resembling that o...
On the basis of anomalous isotopic compositions of oxygen and magnesium, 14 oxide grains from two pr...
Carbonaceous chondrites contain a mixture of solar system condensates, presolar grains, and primitiv...
We report the structural and chemical analyses of six presolar silicate grains identified in situ in...
Raster ion imaging of the oxygen isotopes with the NanoSIMS ion microprobe has been used to identify...
We report the light to intermediate-mass element abundances as well as the oxygen, magnesium, silico...
International audienceAs the chemical compositions of CI chondrites closely resemble that of the Sun...
2 We report the identification of presolar silicates (~177 ppm), presolar oxides (~11 ppm), and one ...
Carbonaceous chondrites contain a mixture of solar system condensates, pre-solar grains, and primiti...
International audienceWe report microscopic, cathodoluminescence, chemical, and O isotopic measureme...
We investigated the inventory of presolar silicate, oxide, and silicon carbide (SiC) grains of fine-...
Abstract—With a new type of ion microprobe, the NanoSIMS, we determined the oxygen isotopic compo-si...
Abstract We investigated the inventory of presolar silicate, oxide, and silicon carbide (SiC) grains...
The majority of presolar silicate and oxide grains derive from low-mass red giant and asymptotic gia...
Presolar oxide grains have been previously divided into several groups (Group 1 to 4) based on their...
International audienceCI chondrites have nonvolatile chemical compositions closely resembling that o...
On the basis of anomalous isotopic compositions of oxygen and magnesium, 14 oxide grains from two pr...
Carbonaceous chondrites contain a mixture of solar system condensates, presolar grains, and primitiv...
We report the structural and chemical analyses of six presolar silicate grains identified in situ in...
Raster ion imaging of the oxygen isotopes with the NanoSIMS ion microprobe has been used to identify...
We report the light to intermediate-mass element abundances as well as the oxygen, magnesium, silico...
International audienceAs the chemical compositions of CI chondrites closely resemble that of the Sun...
2 We report the identification of presolar silicates (~177 ppm), presolar oxides (~11 ppm), and one ...
Carbonaceous chondrites contain a mixture of solar system condensates, pre-solar grains, and primiti...
International audienceWe report microscopic, cathodoluminescence, chemical, and O isotopic measureme...
We investigated the inventory of presolar silicate, oxide, and silicon carbide (SiC) grains of fine-...
Abstract—With a new type of ion microprobe, the NanoSIMS, we determined the oxygen isotopic compo-si...
Abstract We investigated the inventory of presolar silicate, oxide, and silicon carbide (SiC) grains...
The majority of presolar silicate and oxide grains derive from low-mass red giant and asymptotic gia...
Presolar oxide grains have been previously divided into several groups (Group 1 to 4) based on their...
International audienceCI chondrites have nonvolatile chemical compositions closely resembling that o...
On the basis of anomalous isotopic compositions of oxygen and magnesium, 14 oxide grains from two pr...