Zobrazeno 1 - 10
of 118
pro vyhledávání: '"Christine Floss"'
Publikováno v:
Meteoritics & Planetary Science. 55:1228-1256
Publikováno v:
Meteoritics & Planetary Science. 55:1349-1370
Autor:
Dennis Harries, Christian Vollmer, Jan Leitner, Christine Floss, Pierre Haenecour, Peter Hoppe, Knut Metzler, János Kodolányi
Publikováno v:
Meteoritics & Planetary Science. 55:1176-1206
Publikováno v:
Meteoritics & Planetary Science. 55:1207-1227
NASA Cosmochemistry and Emerging Worlds Programs [NNX12AL47G, NNX15AJ22G, 80NSSC19K0509, NNX14AG25G]; McDonnell Center for Space Sciences; NASANational Aeronautics & Space Administration (NASA) [NNX12AL47G, NNX15AJ22G]; NSFNational Science Foundation
Autor:
Christine Floss, David N. Seidman, Dieter Isheim, Tyrone L. Daulton, Ryan C. Ogliore, J. B. Lewis
Publikováno v:
Meteoritics & Planetary Science. 55:1382-1403
Autor:
Christine Floss, Pierre Haenecour, T. K. Croat, Alian Wang, P. K. Carpenter, Thomas J. Zega, Bradley L. Jolliff
Publikováno v:
Geochimica et Cosmochimica Acta. 221:379-405
To investigate the origin of fine-grained rims around chondrules (FGRs), we compared presolar grain abundances, elemental compositions and mineralogies in fine-grained interstitial matrix material and individual FGRs in the primitive CO3.0 chondrites
Publikováno v:
Geochimica et Cosmochimica Acta. 221:255-274
We report the light to intermediate-mass element abundances as well as the oxygen, magnesium, silicon, and titanium isotope compositions of a unique and unusually large (0.8 µm × 3.75 µm) presolar O-rich grain from the Krymka LL3.2 chondrite. The
Publikováno v:
Geochimica et Cosmochimica Acta. 221:237-254
Meteoritic nanodiamonds carry noble gases with anomalies in their stable isotopes that have drawn attention to their potentially presolar origin. Measurements of 12C/13C isotope ratios of presolar nanodiamonds are essential to understanding their ori
Publikováno v:
Earth and Planetary Science Letters. 434:117-128
Carbonaceous chondrites are fragments from primitive parent asteroids, which represent some of the most primitive meteorites accessible for laboratory analysis and offer therefore the best opportunity to explore the chemical and physical conditions i
Autor:
Pierre Haenecour, Christine Floss
Publikováno v:
GEOCHEMICAL JOURNAL. 50:3-25