Size discontinuity between interstellar and chondritic aromatic structures: A high-resolution transmission electron microscopy study

[1]  C. Snape,et al.  Hydropyrolysis of insoluble carbonaceous matter in the Murchison meteorite , 2004 .

[2]  I. Ciofini,et al.  Occurence of abundant diradicaloid moieties in the insoluble organic matter from the Orgueil and Murchison meteorites : a fingerprint of its extraterrestrial origin ? , 2004 .

[3]  Ian Wright,et al.  Investigating the variations in carbon and nitrogen isotopes in carbonaceous chondrites , 2003 .

[4]  S. Derenne,et al.  Heterogeneous distribution of paramagnetic radicals in insoluble organic matter from the Orgueil and Murchison meteorites , 2002 .

[5]  A. Kearsley,et al.  Clay mineral‐organic matter relationships in the early solar system , 2002 .

[6]  R. Saykally,et al.  Single-Photon Infrared Emission Spectroscopy of Gaseous Polycyclic Aromatic Hydrocarbon Cations: A Direct Test for Proposed Carriers of the Unidentified Infrared Emission Bands , 2002 .

[7]  F. Robert.  Water and organic matter D/H ratios in the solar system: a record of an early irradiation of the nebula? , 2002 .

[8]  J. Rouzaud,et al.  Quantitative high-resolution transmission electron microscopy: a promising tool for carbon materials characterization , 2002 .

[9]  George D. Cody,et al.  Solid-state ( 1 H and 13 C) nuclear magnetic resonance spectroscopy of insoluble organic residue in the Murchison meteorite: a self-consistent quantitative analysis , 2002 .

[10]  J. Rouzaud,et al.  Evaluation of a protocol for the quantification of black carbon in sediments , 2001 .

[11]  S. Sandford,et al.  Assessment of the interstellar processes leading to deuterium enrichment in meteoritic organics , 2001 .

[12]  R. Saykally,et al.  Single photon infrared emission spectroscopy of the gas phase pyrene cation: support for a polycyclic aromatic hydrocarbon origin of the unidentified infrared emission bands. , 2001, Physical review letters.

[13]  N. Herlin‐Boime,et al.  Optical properties of synthetic carbon nanoparticles as model of cosmic dust. , 2001, Spectrochimica acta. Part A, Molecular and biomolecular spectroscopy.

[14]  J. Greenberg,et al.  UV photodestruction of CH bonds and the evolution of the 3.4 mu m feature carrier. II. The case of hydrogenated carbon grains , 2001 .

[15]  S. Derenne,et al.  Solid state CP/MAS 13 C NMR of the insoluble organic matter of the Orgueil and Murchison meteorites: quantitative study , 2000 .

[16]  R. Saykally,et al.  Peripherally Hydrogenated Neutral Polycyclic Aromatic Hydrocarbons as Carriers of the 3 Micron Interstellar Infrared Emission Complex: Results from Single-Photon Infrared Emission Spectroscopy , 2000, The Astrophysical journal.

[17]  Pascale Ehrenfreund,et al.  A voyage from dark clouds to the early Earth , 2000 .

[18]  M. Sephton,et al.  Aromatic Moieties in Meteorites: Relics of Interstellar Grain Processes? , 2000 .

[19]  T. Nakagawa,et al.  Unidentified Infrared Emission Bands in the Diffuse Interstellar Medium , 2000, astro-ph/0008335.

[20]  A. Brearley.  Origin of graphitic carbon and pentlandite in matrix olivines in the Allende meteorite. , 1999, Science.

[21]  B. Dubrulle,et al.  Structure and Transport in the Solar Nebula from Constraints on Deuterium Enrichment and Giant Planets Formation , 1999 .

[22]  H. Baumgärtel,et al.  Structure-dependent Photostability of Polycyclic Aromatic Hydrocarbon Cations: Laboratory Studies and Astrophysical Implications , 1999 .

[23]  S. Sandford,et al.  Modeling the Unidentified Infrared Emission with Combinations of Polycyclic Aromatic Hydrocarbons , 1999, The Astrophysical journal.

[24]  Mark A. Sephton,et al.  δ13C of free and macromolecular aromatic structures in the murchison meteorite , 1998 .

[25]  J. Rouzaud,et al.  Nanoparticles produced by Laser Pyrolysis of hydrocarbons: analogy with carbon cosmic dust , 1998 .

[26]  J. Najita,et al.  X-Ray Ionization of Protoplanetary Disks , 1997 .

[27]  J. Rouzaud,et al.  A COMPARISON OF SOLID-STATE CARBONACEOUS MODELS OF COSMIC DUST , 1996 .

[28]  C. Joblin,et al.  Detection of the overtone of the 3.3 micron emission feature in IRAS 21282+5050 , 1994 .

[29]  R N Zare,et al.  Identification of Complex Aromatic Molecules in Individual Interplanetary Dust Particles , 1993, Science.

[30]  L. Colangeli,et al.  Raman and Infrared Spectra of Polycyclic Aromatic Hydrocarbon Molecules of Possible Astrophysical Interest , 1992 .

[31]  F. Rietmeijer.  PREGRAPHITIC AND POORLY GRAPHITISED CARBONS IN POROUS CHONDRITIC MICROMETEORITES , 1992 .

[32]  W. Duley,et al.  Simple linear polycyclic aromatic hydrocarbon molecules and the infrared emission features - Mothballs in the Orion ridge , 1990 .

[33]  A. Tielens,et al.  Interstellar polycyclic aromatic hydrocarbons: the infrared emission bands, the excitation/emission mechanism, and the astrophysical implications. , 1989, The Astrophysical journal. Supplement series.

[34]  T. Wdowiak,et al.  Insoluble organic material of the Orgueil carbonaceous chondrite and the unidentified infrared bands. , 1988, The Astrophysical journal.

[35]  S. Sandford,et al.  Interstellar Polycyclic Aromatic Hydrocarbons and Carbon in Interplanetary Dust Particles and Meteorites , 1987, Science.

[36]  Frans J. M. Rietmeijer,et al.  Metastable carbon in two chondritic porous interplanetary dust particles , 1987, Nature.

[37]  T. Miyata,et al.  Primary structure of the α-subunit of Torpedo californica (Na+ + K+)ATPase deduced from cDNA sequence , 1985, Nature.

[38]  Frans J. M. Rietmeijer,et al.  Poorly graphitized carbon as a new cosmothermometer for primitive extraterrestrial materials , 1985, Nature.

[39]  Alexander G. G. M. Tielens,et al.  Polycyclic aromatic hydrocarbons and the unidentified infrared emission bands - Auto exhaust along the Milky Way , 1985 .

[40]  J. Puget,et al.  Identification of the 'unidentified' IR emission features of interstellar dust? , 1984 .

[41]  S. Pizzarello,et al.  13C NMR spectroscopy of the insoluble carbon of carbonaceous chondrites. , 1982, Geochimica et cosmochimica acta.

[42]  P. Buseck,et al.  Graphitic carbon in the Allende meteorite: a microstructural study. , 1981, Science.

[43]  T. E. Bunch,et al.  Carbonaceous chondrites. II - Carbonaceous chondrite phyllosilicates and light element geochemistry as indicators of parent body processes and surface conditions , 1980 .

[44]  Sumiko Matsuoka,et al.  Origin of organic matter in the early solar system—VII. The organic polymer in carbonaceous chondrites , 1977 .

[45]  P. Raynal.  Etude en laboratoire de matière extraterrestre : implications pour la physico-chimie du Système Solaire primitif , 2003 .

[46]  N. Herlin‐Boime,et al.  Carbon nanoparticles from laser pyrolysis , 2002 .

[47]  Y. Pendleton,et al.  The Organic Refractory Material in the Diffuse Interstellar Medium: Mid-Infrared Spectroscopic Constraints , 2002 .

[48]  R. Hurt,et al.  A methodology for analysis of 002 lattice fringe images and its application to combustion-derived carbons , 2000 .

[49]  C. T. Pillinger,et al.  Aromatic moieties in meteoritic macromolecular materials: analyses by hydrous pyrolysis and δ13C of individual compounds , 2000 .

[50]  L. Allamandola.  INTERSTELLAR POLYCYCLIC AROMATIC HYDROCARBONS , 1999 .

[51]  L. Colangeli,et al.  IDENTIFICATION OF CARBON FORMS IN SOOT MATERIALS OF ASTROPHYSICAL INTEREST , 1998 .

[52]  T. Zheng.  Quantitative high resolution transmission electron microscopy , 1995 .

[53]  S. Tobita,et al.  SIZE EFFECTS ON DISSOCIATION RATES OF POLYCYCLIC AROMATIC HYDROCARBON CATIONS : LABORATORY STUDIES AND ASTROPHYSICAL IMPLICATIONS , 1994 .

[54]  P. Ehrenfreund,et al.  Similarity of the infrared spectrum of an Orgueil organic polymer with interstellar organic compounds in the line of sight towards IRS 7. , 1992, Advances in space research : the official journal of the Committee on Space Research.

[55]  F. Rietmeijer.  Mixed layering in disordered Sri Lanka graphite , 1991 .

[56]  H. Charcosset,et al.  Advanced methodologies in coal characterization , 1990 .

[57]  J. Rouzaud.  Contribution of transmission electron microscopy to the study of the coal carbonization processes , 1990 .

[58]  J. Rouzaud,et al.  The characterization of coals and cokes by transmission electron microscopy , 1990 .

[59]  T. Geballe,et al.  Polycyclic aromatic hydrocarbons in the near-infrared spectra of 24 IRAS sources , 1990 .

[60]  J. Puget,et al.  A New Component of the Interstellar Matter: Small Grains and Large Aromatic Molecules , 1989 .

[61]  J. Rouzaud,et al.  Structure, microtexture, and optical properties of anthracene and saccharose-based carbons , 1989 .

[62]  L. Reimer,et al.  Scanning Electron Microscopy , 1984 .

[63]  P. Buseck,et al.  Carbon in the Allende meteorite - Evidence for poorly graphitized carbon rather than carbyne , 1982 .