ISOTOPIC ANOMALIES IN PRIMITIVE SOLAR SYSTEM MATTER: SPIN-STATE-DEPENDENT FRACTIONATION OF NITROGEN AND DEUTERIUM IN INTERSTELLAR CLOUDS
- 4 September 2012
- journal article
- Published by American Astronomical Society in The Astrophysical Journal Letters
- Vol. 757 (1), L11
- https://doi.org/10.1088/2041-8205/757/1/l11
Abstract
No abstract availableKeywords
This publication has 44 references indexed in Scilit:
- AMMONIA IN THE EARLY SOLAR SYSTEM: AN ACCOUNT FROM CARBONACEOUS METEORITESThe Astrophysical Journal, 2012
- Nitrogen hydrides and the H2ortho-to-para ratio in dark cloudsAstronomy & Astrophysics, 2011
- The Chemical Composition of Comets—Emerging Taxonomies and Natal HeritageAnnual Review of Astronomy and Astrophysics, 2011
- Detection of N$^\mathsf{{15}}$NH+in L1544Astronomy & Astrophysics, 2010
- Pristine extraterrestrial material with unprecedented nitrogen isotopic variationProceedings of the National Academy of Sciences of the United States of America, 2009
- Enrichment of deuterium in insoluble organic matter from primitive meteorites: A solar system origin?Earth and Planetary Science Letters, 2006
- Complete depletion in prestellar coresAstronomy & Astrophysics, 2004
- The End of Interstellar Chemistry as the Origin of Nitrogen in Comets and MeteoritesThe Astrophysical Journal, 2002
- The possibility of nitrogen isotopic fractionation in interstellar cloudsMonthly Notices of the Royal Astronomical Society, 2000
- Reactions of H2 with He+ at temperatures below 40 KThe Journal of Chemical Physics, 1989