Presolar stardust in meteorites : recent advances and scientific frontiers

By L. Nittler. 2003

189 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/523a030f965c30c30f4c75041b76ea6c4b8e006b

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In Astronomy and Astrophysics

Citations in the corpus

Ultra-primitive interplanetary dust particles from the comet 26P/Grigg–Skjellerup dust stream collection (2009, background): “The seven 17O-rich (“Group1”) grains likely formed inwinds of lowmass asymptotic giant branch stars (Nittler, 2003),whereas the origin of the four 17O-depleted (“Group 3”, Nittler, 1997) grains is more ambiguous.”
Origin of the Chemical Elements (2010, background): “There are a number of excellent reviews on the topic (e.g. Nittler 2003, Clayton and Nittler 2004, Zinner et al. 2006, and the book by Lugaro 2005).”
Characterization of Presolar Silicate and Oxide Grains in Primitive Carbonaceous Chondrites (2007, background): “Dust grains that condensed in the atmospheres of evolved stars and in nova and supernova ejecta are preserved in primitive meteorites, interplanetary dust particles (IDPs), and Antarctic micrometeorites (AMMs; Nittler 2003; Zinner 2004; Yada et al. 2005, 2006).”
Molybdenum isotope anomalies in meteorites: Constraints on solar nebula evolution and origin of the Earth (2011, background): “Some of the diverse nucleosynthetic components that +41 44 63 21827. rdt). l rights reserved. contributed material to the solar system have been identified via presolar grains in primitive chondrites (e.g., Nittler, 2003).”
Astrophysics with Presolar Stardust (2004, background): “Quite a large literature exists documenting the discovery of presolar stardust and their scientific consequences, including recent reviews by Zinner (1998) and Nittler (2003).”
Stable-isotopic anomalies and the accretionary assemblage of the Earth and Mars: A subordinate role for carbonaceous chondrites (2011, background): “Presolar grains are trace components and rarely feature 16O enrichment (Nittler, 2003), so origin of the Δ17O diversity was clearly not tied to presolar nanoparticles of the type found by Zinner et al. (2005) (cf. Dauphas et al., 2010).”