Astrophysics with Presolar Stardust

By D. Clayton, L. Nittler. 2004

242 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/a25439a457245a227a7e010c2033cac8e17e8306

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

Citations in the corpus

The s process: Nuclear physics, stellar models, and observations (2010, background): “In addition, information on individual nucleosynthesis events are provided by the rapid progress in the measurements on pre-solar grains, which provide accurate isotope ratios of important elements (Clayton and Nittler, 2004; Nittler, 2009; Zinner, 1998).”
THE DISCOVERY AND ANALYSIS OF VERY METAL-POOR STARS IN THE GALAXY (2005, background): “Detailed measurements of individual isotopes are now routinely obtained from the analysis of solar-system material, such as in meteorites (see, e.g., Clayton & Nittler 2004).”
GALACTIC CHEMICAL EVOLUTION AND SOLAR s-PROCESS ABUNDANCES: DEPENDENCE ON THE 13C-POCKET STRUCTURE (2014, background): “A similar spread is shown by s-process isotopic signatures found in presolar meteoritic SiC grains, which originated in the outflow of AGB stars (see, e.g., Lugaro et al. 2003; Clayton & Nittler 2004; Zinner 2007).”
NUGRID STELLAR DATA SET. I. STELLAR YIELDS FROM H TO BI FOR STARS WITH METALLICITIES Z = 0.02 and Z = 0.01 (2013, background): “These carry a relatively unmodified nucleosynthesis signature from the environment of their parent stars (e.g., Zinner 2003; Clayton & Nittler 2004).”
Chondrules and the Protoplanetary Disk (2011, background): “However, this explanation is no longer favored as stardust is largely 17O-rich and CAIs do not show comparable anomalies in other elements (Clayton & Nittler 2004).”
The 12C/13C Isotope Gradient Derived from Millimeter Transitions of CN: The Case for Galactic Chemical Evolution (2005, background): “The abundance ratio range is set by the bulk values found for meteorites, comets, and interplanetary dust particles ( IDPs), 12C/13C ¼ 89 1 (Clayton & Nittler 2004).”
Dust formation and survival in supernova ejecta (2007, background): “SiC grains, found in meteorites and considered to be of SN origin from their anomalous isotopic ratios (Clayton & Nittler 2004), are not considered since their formation is impeded by the formation of AC and Si-bearing grains (Nozawa et al. 2003).”
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).”