Presolar grains are nanometer- to micrometer-sized dust grains that are found in small quantities in primitive meteorites , interplanetary dust particles (IDPs), and in cometary matter. They are older than our Solar System and formed in the winds of evolved stars and in the ejecta of stellar explosions, as evidenced by large isotopic abundance anomalies
Many meteorites contain small quantities of microscopic particles with unusual mixes of isotopes. Th...
Isotopic studies of IDPs collected from the comet Grigg-Skjellerup dust stream reveal extremely high...
Primitive Solar System materials host small amounts of refractory dust grains predating the formatio...
Presolar grains are nanometer- to micrometer-sized dust grains that are found in small quantities in...
This work is part of an ongoing investigation [1-3] of isotopically anomalous phases in interplaneta...
Primitive Solar System materials, such as certain types of meteorites, interplanetary dust particles...
Pristine stardust grains from the interstellar gas and dust cloud from which our Solar System formed...
Grains of stardust that formed in stellar outflows prior to the formation of the solar system surviv...
The study of presolar meteoritic grains is a new inter-disciplinary field that brings together topic...
Primitive solar system materials, namely, meteorites, interplanetary dust particles, and cometary ma...
Primitive meteorites contain small quantities of presolar grains with highly anomalous isotopic comp...
Primitive meteorites and interplanetary dust particles contain presolar grains: pristine solid sampl...
The time span between the formation of presolar grains in stellar outflows and their incorporation i...
Abstract. Solid particles, usually referred to as dust, are a crucial component of inter-stellar mat...
Raster ion imaging of the oxygen isotopes with the NanoSIMS ion microprobe has been used to identify...
Many meteorites contain small quantities of microscopic particles with unusual mixes of isotopes. Th...
Isotopic studies of IDPs collected from the comet Grigg-Skjellerup dust stream reveal extremely high...
Primitive Solar System materials host small amounts of refractory dust grains predating the formatio...
Presolar grains are nanometer- to micrometer-sized dust grains that are found in small quantities in...
This work is part of an ongoing investigation [1-3] of isotopically anomalous phases in interplaneta...
Primitive Solar System materials, such as certain types of meteorites, interplanetary dust particles...
Pristine stardust grains from the interstellar gas and dust cloud from which our Solar System formed...
Grains of stardust that formed in stellar outflows prior to the formation of the solar system surviv...
The study of presolar meteoritic grains is a new inter-disciplinary field that brings together topic...
Primitive solar system materials, namely, meteorites, interplanetary dust particles, and cometary ma...
Primitive meteorites contain small quantities of presolar grains with highly anomalous isotopic comp...
Primitive meteorites and interplanetary dust particles contain presolar grains: pristine solid sampl...
The time span between the formation of presolar grains in stellar outflows and their incorporation i...
Abstract. Solid particles, usually referred to as dust, are a crucial component of inter-stellar mat...
Raster ion imaging of the oxygen isotopes with the NanoSIMS ion microprobe has been used to identify...
Many meteorites contain small quantities of microscopic particles with unusual mixes of isotopes. Th...
Isotopic studies of IDPs collected from the comet Grigg-Skjellerup dust stream reveal extremely high...
Primitive Solar System materials host small amounts of refractory dust grains predating the formatio...
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