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Stardust@home

Known as: Stardust 
Stardust@home is a citizen science project that encourages volunteers to search images for tiny interstellar dust impacts. The project began… Expand
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Papers overview

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2018
2018
About 30%–40% of classical novae produce dust 20–100 days after the outburst, but no presolar stardust grains from classical… Expand
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2014
2014
We discuss the inherent difficulties that arise during "ground truth" characterization of the Stardust interstellar dust… Expand
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2013
2013
Glycine (C2H5NO2) was the first amino acid to be detected in space by the stardust space probe in Comet Wild2, and is used by… Expand
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2013
2013
We present model predictions for the Zr isotopic ratios produced by slow neutron captures in C-rich asymptotic giant branch (AGB… Expand
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2009
2009
Introduction: Presolar material incorporated into primitive solar system bodies consists of both circumstellar stardust formed in… Expand
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Highly Cited
2009
Highly Cited
2009
Abstract We have investigated the presolar grain inventories of two CR chondrites, QUE 99177 and MET 00426, which are less… Expand
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Highly Cited
2008
Highly Cited
2008
Aims. We studied the evolution of the abundance in interstellar dust species that originate in stellar sources and from… Expand
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Highly Cited
2003
Highly Cited
2003
Grains of stardust that formed in stellar outflows prior to the formation of the solar system survive intact as trace… Expand
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1999
1999
Observational and theoretical studies of the outbursts of classical novae have provided critical insights into a broad range of… Expand
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Highly Cited
1997
Highly Cited
1997
Thirty-seven isotopically highly anomalous presolar Al2O3 grains and one presolar MgAl2O4 grain from a separate of the Tieschitz… Expand
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