Zobrazeno 1 - 10
of 18
pro vyhledávání: '"Manavi Jadhav"'
Autor:
Rainer Wieler, Matthias M. M. Meier, Henner Busemann, Colin Maden, Heinrich Baur, Philipp R. Heck, Ernst Zinner, Frank Gyngard, Sachiko Amari, Manavi Jadhav, Teruyuki Maruoka
Publikováno v:
Meteoritics & Planetary Science. 53:2327-2342
We present He and Ne isotopes of individual presolar graphite grains from a low-density separate from Orgueil. Two grain mounts were analyzed with the same techniques but in a different sequence: The first one was measured with NanoSIMS followed by n
Autor:
Reto Trappitsch, Peter Hoppe, Manavi Jadhav, Nicolas Dauphas, Christopher H. Kelly, Frank Gyngard, Detlef Rost, Thomas Stephan, Michael J. Pellin, Andrew M. Davis, Michael R. Savina
Publikováno v:
Geochimica et Cosmochimica Acta. 221:109-126
We used CHILI, the Chicago Instrument for Laser Ionization, a new resonance ionization mass spectrometer developed for isotopic analysis of small samples, to analyze strontium, zirconium, and barium isotopes in 22 presolar silicon carbide grains. Twe
Publikováno v:
Geochimica et Cosmochimica Acta. 221:60-86
We report the morphology, microstructure, and isotopic composition of the largest SiC stardust grain known to have condensed from a supernova. The 25-μm diameter grain, termed Bonanza, was found in an acid-resistant residue of the Murchison meteorit
Publikováno v:
Geological Society of America Abstracts with Programs.
Autor:
Kuljeet K. Marhas, Sachiko Amari, Teruyuki Maruoka, Ernst Zinner, Manavi Jadhav, Roberto Gallino
Publikováno v:
Geochimica et Cosmochimica Acta. 113:193-224
We report C, N, O, Si, Al–Mg, K, Ca, and Ti isotopic analyses of presolar graphite grains from the Orgueil CI chondrite. NanoSIMS isotopic measurements were made on 345 grains from seven density fractions, with grain sizes >1 lm: low-density grains
Publikováno v:
Meteoritics & Planetary Science. 48:686-699
Transmission electron microscope (TEM) investigations have revealed Os, Ru, Mo-rich refractory metal nuggets within four different presolar graphites, from both the high-density (HD) Murchison (MUR) and low-density (LD) Orgueil (ORG) fractions. Micro
Autor:
Roberto Gallino, Teruyuki Maruoka, Ernst Zinner, Manavi Jadhav, Sachiko Amari, Kuljeet K. Marhas
Publikováno v:
The Astrophysical Journal. 682:1479-1485
WepresentC,N,O,Si,Al-Mg,K,Ca,andTiisotopicanalyses ofsevenhigh-density(ORG1f, � � 2:02 2:04 gcm � 3 ) graphite grains from Orgueil with 12 C/ 13 C ratios smaller than 20. The presence of 44Ti in three of these grains indicates an origin in Type
Publikováno v:
Proceedings of XIII Nuclei in the Cosmos — PoS(NIC XIII).
Publikováno v:
New Astronomy Reviews. 50:591-595
We report the successful isolation and isotopic analysis of presolar graphite grains from the Orgueil CI chondrite. Isotopic measurements were made on seven density fractions, with grain sizes >1 μm: ORG1b (1.59–1.67 g cm −3 ), 1c (1.67–1.75 g
Publikováno v:
ASTROPHYSICAL JOURNAL LETTERS
ApJ Letters
ApJ Letters
Graphite is one of the many presolar circumstellar condensate species found in primitive meteorites. While the isotopic compositions of low-density graphite grains indicate an origin in core-collapse supernovae, some high-density grains have extreme
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e14190504d4c9b6aa44f3b3721b8e73a
http://arxiv.org/abs/1310.2679
http://arxiv.org/abs/1310.2679