Characterization of Presolar Silicate and Oxide Grains in Primitive Carbonaceous Chondrites

By A. Nguyen, F. Stadermann, E. Zinner, R. Stroud, C. Alexander, L. Nittler. 2007

142 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Ecology, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/b24a44523d4eba4aed45e1fc8ac1b882c74bb03b

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

1. L. Nittler
2. F. Ciesla
3. Cecilia Ceccarelli
4. P. Caselli
5. S. Zhukovska
6. M. Trieloff
7. C. Alexander
8. A. Nguyen

In Ecology

1. Roberto Gallino
2. Cecilia Ceccarelli
3. P. Caselli
4. E. Zinner
5. C. Alexander

In Spectroscopy

1. Cecilia Ceccarelli
2. P. Caselli
3. A. Jones
4. L. Nittler
5. C. Alexander

Citations in the corpus

• NanoSIMS: Technical Aspects and Applications in Cosmochemistry and Biological Geochemistry (2013, unknown): “Primitive meteorites and Antarctic micrometeorites show lower presolar silicate abundances (Nguyen et al. 2007, 2010b, Yada et al. 2008, Floss and Stadermann 2009, Vollmer et al. 2009, Bose et al. 2010, Leitner et al. 2012).”
• Aluminum-, Calcium- and Titanium-rich Oxide Stardust in Ordinary Chondrite Meteorites (2008, background): “…of manymore presolar spinel grains (Zinner et al. 2003) and, more significantly, the discovery and characterization of presolar silicate minerals (Floss et al. 2006; Messenger et al. 2003; Mostefaoui & Hoppe 2004; Nagashima et al. 2004; Nguyen et al. 2007; Nguyen& Zinner 2004; Vollmer et al. 2007).”
• Astrophysics with Extraterrestrial Materials (2016, background): “…crystallinity, purely amorphous grains with nonstoichiometric compositions that are sometimes spatially heterogeneous on a scale of tens of nanometers, and others (Messenger et al. 2005; Nguyen et al. 2007, 2010; Vollmer et al. 2007, 2009, 2013; Keller & Messenger 2011; Stroud et al. 2013, 2014).”
• The evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point (2013, background): “Secondly, they appear to be consistent with the sizes of the pre-solar amorphous and crystalline silicate grains of evolved star origin that have been analysed in meteorites (e.g., Nguyen et al. 2007).”
• Our astrochemical heritage (2012, background): “Such Fe-rich grains may be due to a secondary alteration of the disk mineralogy (see also Nguyen et al. 2007), probably originated within large differentiated bodies (as in the case of the S-type asteroid recently studied with the Hayabusa re-entry module; Nakamura et al. 2011).”
• Evolution of interstellar dust and stardust in the solar neighbourhood (2007, background): “The number of silicate grains from stellar sources detected in meteorites and interplanetary dust particles has been small up to now (Nguyen et al. 2007; Messenger et al. 2005).”
• Ultra-primitive interplanetary dust particles from the comet 26P/Grigg–Skjellerup dust stream collection (2009, background): “, 2006), and 100 to 200 ppm in themost presolar grain-rich meteorites, the carbonaceous chondrites Acfer 094, Meteorite Hills 00426 and Queen Elizabeth Range 99177 (Nguyen et al., 2007; Vollmer et al., 2008; Floss and Stadermann, 2009).”