View Item 

Show simple item record

Oxygen isotope anomalies of the Sun and the original environment of the solar system
dc.contributor.authorLee, Jeong‐eunen_US
dc.contributor.authorBergin, Edwin A.en_US
dc.contributor.authorLyons, James R.en_US
dc.date.accessioned2013-03-05T18:17:28Z
dc.date.available2013-03-05T18:17:28Z
dc.date.issued2008-08en_US
dc.identifier.citationLee, Jeong‐eun ; Bergin, Edwin A. ; Lyons, James R. (2008). "Oxygen isotope anomalies of the Sun and the original environment of the solar system." Meteoritics & Planetary Science 43(8). <http://hdl.handle.net/2027.42/96691>en_US
dc.identifier.issn1086-9379en_US
dc.identifier.issn1945-5100en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/96691
dc.publisherBlackwell Publishing Ltden_US
dc.publisherWiley Periodicals, Inc.en_US
dc.titleOxygen isotope anomalies of the Sun and the original environment of the solar systemen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAstronomy and Astrophysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Astronomy, The University of Michigan, 500 Church Street, Ann Arbor, Michigan 48109‐10424en_US
dc.contributor.affiliationotherDepartment of Earth and Space Sciences, University of California, Los Angeles, California 90095, USAen_US
dc.contributor.affiliationotherInstitute of Geophysics and Planetary Physics, University of California, Los Angeles, California 90095, USAen_US
dc.contributor.affiliationotherPhysics and Astronomy Department, The University of California at Los Angeles, PAB, Box 951547, Los Angeles, California 90095‐1547, USAen_US
dc.contributor.affiliationotherDepartment of Astronomy and Space Science, Astrophysical Research Center for the Structure and Evolution of the Cosmos, Sejong University, Seoul 143‐747, Koreaen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/96691/1/j.1945-5100.2008.tb00702.x.pdf
dc.identifier.doi10.1111/j.1945-5100.2008.tb00702.xen_US
dc.identifier.sourceMeteoritics & Planetary Scienceen_US
dc.identifier.citedreferenceParravano A., Hollenbach D. J., and McKee C. F. 2003. Time dependence of the ultraviolet radiation field in the local interstellar medium. The Astrophysical Journal 584: 797.en_US
dc.identifier.citedreferenceIreland T. R., Holden P., Norman M. D., and Clark J. 2006. Isotopic enhancements of 17 O and 18 O from solar wind particles in the lunar regolith. Nature 440: 776 – 778.en_US
dc.identifier.citedreferenceKobayashi S., Imai H., and Yurimoto H. 2003. New extreme 16 O‐rich reservoir in the early solar system. Geochemical Journal 37: 663 – 669.en_US
dc.identifier.citedreferenceLee J.‐E., Bergin E. A., and Evans N. J. II 2004. Evolution of chemistry and molecular line profiles during protostellar collapse. The Astrophysical Journal 617: 360 – 384.en_US
dc.identifier.citedreferenceLyons J. R. and Young E. D. 2005. CO self‐shielding as the origin of oxygen isotope anomalies in the early solar nebula. Nature 435: 317 – 320.en_US
dc.identifier.citedreferenceMcKeegan K. D., Jarzebinski G., Kallio A. P., Mao P. H., Coath C. D., Kunihiro T., Wiens R., Allton J., Callaway M., Rodriguez M., and Burnett D. S. 2008. A first look at oxygen in a Genesis concentrator sample (abstract #2020). 39th Lunar and Planetary Science Conference. CD‐ROM.en_US
dc.identifier.citedreferenceMillar T. J., Farquhar P. R. A., and Willacy K. 1997. The UMIST Database for Astrochemistry. Astronomy and Astrophysics Supplement 121: 139 – 185.en_US
dc.identifier.citedreferenceÖberg K. I., Fuchs G. W., Awad Z., Fraser H. J., Schlemmer S., Van Dishoeck E. F., and Linnartz H. 2007. Photodesorption of CO ice. The Astrophysical Journal 662: L23 – L26.en_US
dc.identifier.citedreferenceOuellette N., Desch S. J., Hester J. J., and Leshin L. A. 2005. A nearby supernova injected short‐lived radionuclides into our protoplanetary disk. In Chondrites and the protoplanetary disk, edited by Krot A. N., Scott E. R. D., and Reipurth B. Astronomical Society of the Pacific Conference Series, vol. 431. pp. 527 – 538.en_US
dc.identifier.citedreferenceSakamoto N., Seto Y., Itoh S., Kuramoto K., Fujino K., Nagashima K., Krot A. N., and Yurimoto H. 2007. Remnants of the early solar system water enriched in heavy oxygen isotopes. Science 317: 231 – 233.en_US
dc.identifier.citedreferenceShu F. H. 1977. Self‐similar collapse of isothermal spheres and star formation. The Astrophysical Journal 214: 488 – 497.en_US
dc.identifier.citedreferenceShukolyukov A. and Lugwair G. W. 1993. Live iron‐60 in the early solar system. Science 259: 1138 – 1142.en_US
dc.identifier.citedreferenceTachibana S. and Huss G. R. 2003. The initial abundance of 60 Fe in the solar system. The Astrophysical Journal Letters 588: 41 – 44.en_US
dc.identifier.citedreferenceTerebey S., Shu F. H., and Cassen P. 1984. The collapse of the cores of slowly rotating isothermal clouds. The Astrophysical Journal 286: 529 – 551.en_US
dc.identifier.citedreferenceVan Boekel R. M., Min M., Leinert Ch., Waters L. B. F. M., Richichi A., Chesneau O., Dominik C., Jaffe W., Dutrey A., Graser U., Henning Th., De Jong J., Köhler R., De Koter A., Lopez B., Malbet F., Morel S., Paresce F., Perrin G., Preibisch Th., F. Przygodda F., Schöller M., and Wittkowski M. 2004. The building blocks of planets within the “terrestrial” region of protoplanetary disks. Nature 432: 479 – 482.en_US
dc.identifier.citedreferenceVan Broekhuizen F. 2005. PhD thesis, Leiden University, Leiden, Netherlands. pp. 73 – 104.en_US
dc.identifier.citedreferenceVan Dishoeck E. F. and Black J. H. 1988. The photodissociation and chemistry of interstellar CO. The Astrophysical Journal 334: 771 – 802.en_US
dc.identifier.citedreferenceWadhwa M., Amelin Y., Davis A. M., Lugmair G. W., Meyer B., Gounelle M., and Desch S. J. 2007. From dust to planetesimals: Implications for the solar protoplanetary disk from short‐lived radionuclides. In Protostars and planets V, edited by Reipurth B., Jewitt D., and Keil K. Tucson: The University of Arizona Press. 1024 p.en_US
dc.identifier.citedreferenceWestley M. S., Baragiola R. A., Johnson R. E., and Baratta G. 1995. Photodesorption from low temperature water ice in interstellar and circumsolar grains. Nature 373: 405 – 407.en_US
dc.identifier.citedreferenceYurimoto H. and Kuramoto K. 2004. Molecular cloud origin for the oxygen isotope heterogeneity in the solar system. Science 305: 1763 – 1766.en_US
dc.identifier.citedreferenceYurimoto H., Kuramoto K., Krot A. N., Scott E. R. D., Cuzzi J. N., Thiemens M. H., and Lyons J. R. Origin and. evolution of oxygen isotopic compositions of the solar system 2007. In Protostars and planets V, edited by Reipurth B., Jewitt D. and Keil K. Tucson: The University of Arizona Press. 1024 p.en_US
dc.identifier.citedreferenceAdams F. C., Hollenbach D., Laughlin G., and Gorti U. 2004. Photoevaporation of circumstellar disks due to external farultraviolet radiation in stellar aggregates. The Astrophysical Journal 611: 360 – 379.en_US
dc.identifier.citedreferencePrieto, Allende C., Lambert D. L., and Asplund M. 2002. A reappraisal of the solar photospheric C/O ratio. The Astrophysical Journal Letters 573: 137 – 140.en_US
dc.identifier.citedreferenceBergin E. A. and Langer W. D. 1997a. Chemical evolution in pre‐protostellar and protostellar cores. The Astrophysical Journal 486: 316 – 328.en_US
dc.identifier.citedreferenceBergin E. A., Goldsmith P. F., Snell R. L., and Langer W. D. 1997b. The chemical composition and evolution of giant molecular cloud cores: A comparison of observation and theory. The Astrophysical Journal 482: 285 – 297.en_US
dc.identifier.citedreferenceBergin E. A., Maret S., Van der Tak F. F. S., Alves J., Carmody S., and Lada C. J. 2006. The thermal structure of gas in prestellar cores: A case study of Barnard 68. The Astrophysical Journal 645: 369 – 380.en_US
dc.identifier.citedreferenceBergin E. A., Aikawa Y., Blake G. A., and Van Dishoeck E. F. 2007. The chemical evolution of disks. In Protostars and planets V, edited by Reipurth B., Jewitt D., and Keil K. Tucson: The University of Arizona Press. 1024 p.en_US
dc.identifier.citedreferenceBlaauw A. 1992. OB associations and the fossil record of star formation. In The physics of star formation and early stellar evolution, edited by Lada C. J. and Kylafis N. D. NATA ASI Series 342. 125 p.en_US
dc.identifier.citedreferenceBonnoer W. B. 1956. Boyle's Law and gravitational instability. Monthly Notices of the Royal Astronomical Society 116: 351 – 359.en_US
dc.identifier.citedreferenceBrownlee D., Tsou P., Aléon J., Alexander C. M. O'D., Araki T., Bajt S., Baratta G. A., Bastien R., Bland P., Bleuet P., Borg J., Bradley J. P., Brearley A., Brenker F., Brennan S., Bridges J. C. Browning N., Brucato J. R., Brucato H., Bullock E., Burchell M. J., Busemann H., Butterworth A., Chaussidon M., Cheuvront A., Chi M., Cintala M. J., Clark B. C., Clemett S. J., Cody G., Colangeli L., Cooper G., Cordier P. G., Daghlian, C., Dai Z., D'Hendecourt L., Djouadi Z., Dominguez G., Duxbury T., Dworkin J. P., Ebel D., Economou T. E., Fairey S. A. J., Fallon S., Ferrini G., Ferroir T. Fleckenstein H., Floss C., Flynn G., Franchi I. A., Fries M., Gainsforth Z., Gallien J.‐P., Genge M., Gilles M. K., Gillet P., Gilmour J., Glavin D. P., Gounelle M., Grady M. M., Graham G. A., Grant P. G., Green S. F., Grossemy F. Grossman L., Grossman J., Guan Y., Hagiya K., Harvey R., Heck P., Herzog G. F., Hoppe P., Hörz F., Huth J., Hutcheon I. D., Ishii H., Ito M., Jacob D., Jacobsen C., Jacobsen S., Joswiak D., Kearsley A. T., Keller L., Khodja H. Kilcoyne A. L. D., Kissel J., Krot A., Langenhorst F., Lanzirotti A., Le L., Leshin L., Leitner J., Lemelle L., Leroux H., Liu M.‐C., Luening K., Lyon I., MacPherson G., Marcus M. A., Marhas K., Matrajt G., Meibom A., Mennella V., Messenger K., Mikouchi T., Mostefaoui S., Nakamura T., Nakano T., Newville M., Nittler L. R., Ohnishi I., Ohsumi K., Okudaira K., Papanastassiou D. A., Palma R., Palumbo M. O., Pepin R, E., Perkins D., Perronnet M., Pianetta P., Rao W., Rietmeijer F., Robert F., Rost D., Rotundi A., Ryan R., Sandford S. A., Schwandt C. S., See, T. H., Schlutter D., Sheffield‐Parker J. A., Simionovici S., Sitnitsky S., I. Snead C. J. Spencer M. K. Stadermann F. J., Steele A., Stephan T., Stroud R., Susini J., Sutton S. R., Taheri M., Taylor S., Teslich N., Tomeoka K., Tomioka N., Toppani A., Trigo‐Rodriguez J. M., Troadec D., Tsuchiyama A., Tuzolino A. J., Tyliszczak, T., Uesugi K., Velbel M., Vellenga J., Vicenzi E., Vincze L., Warren J., Weber I., Weisberg M., Westphal A. J., Wirick S., Wooden D., Wopenka B., Wozniakiewicz P. A., Wright I., Yabuta H., Yano H., Young E. D., Zare R. N., Zega T., Ziegler K., Zimmerman L., Zinner E., and Zolensky M. 2006. Comet Wild 2 under a microscope. Science 314: 1711 – 1716.en_US
dc.identifier.citedreferenceCameron A. G. W. and Truran J. W. 1977. The supernova trigger for formation of the solar system. Icarus 30: 447.en_US
dc.identifier.citedreferenceCiesla F. J. and Cuzzi J. N. 2006. The evolution of the water distribution in a viscous protoplanetary disk. Icarus 181: 178.en_US
dc.identifier.citedreferenceClayton R. N. 2002. Self‐shielding in the solar nebula. Nature 415: 860 – 861.en_US
dc.identifier.citedreferenceCuzzi J. N. and Zahnle K. J. 2004. Material enhancement in protoplanetary nebulae by particle drift through evaporation fronts. The Astrophysical Journal Supplement 614: 490 – 496.en_US
dc.identifier.citedreferenceEcuvillon A., Israelian G., Santos N. C., Mayor M., and Gilli G. 2006. Abundance ratios of volatile versus refractory elements in planet‐harbouring stars: Hints of pollution? Astronomy and Astrophysics 449: 809 – 816.en_US
dc.identifier.citedreferenceEbert R. 1955. Über die Verdichtung von H I‐Gebieten. Mit 5 Textabbildungen. Zeitschrift für Astrophysik 37: 217 – 232.en_US
dc.identifier.citedreferenceEberhardt P., Reber M., Krankowsky D., and Hodges R. R. 1995. The D/H and 18 O/ 16 O ratios in water from comet P/Halley. Astronomy and Astrophysics 302: 301 – 316.en_US
dc.identifier.citedreferenceEvans N. J. II, Rawlings J. M. C., Shirely Y. L., and Mundy L. G. 2001. Tracing the mass during low‐mass star formation. II. modeling the submillimeter emission from pre‐protostellar cores. The Astrophysical Journal 557: 193 – 208.en_US
dc.identifier.citedreferenceFurlan E., Hartmann L., Calvet N., D'Alessio P., Franco‐Hernández R., Forrest W. J., Watson D. M., and Uchida K. I. et al. 2006. A survey and analysis of Spitzer infrared spectrograph spectra of T Tauri stars in Taurus. The Astrophysical Journal Supplement 165: 568 – 605.en_US
dc.identifier.citedreferenceGreenberg J. M. 1973. Photodesorption from interstellar dust grains In International Astronomical Union Symposium No. 52, Interstellar dust and related topics, edited by Greenberg J. M. and Van de Hulst H.C. Dordrecht: Reidel. 584 p.en_US
dc.identifier.citedreferenceGounelle M. 2006. The origin of short‐lived radionuclides in the solar system. New Astronomy Reviews 50: 596.en_US
dc.identifier.citedreferenceHabing H. J. 1968. The interstellar radiation density between 912 A and 2400 A. Bulletin of the Astronomical Institutes of the Netherlands 19: 421 – 431.en_US
dc.identifier.citedreferenceHartmann L. 1998. Accretion processes in star formation. Cambridge: Cambridge University Press. 260 p.en_US
dc.identifier.citedreferenceHashizume K., Chaussidon M., Marty B., and Robert F. 2000. Solar wind record of the Moon: Deciphering presolar from planetary nitrogen. Science 290: 1142 – 45.en_US
dc.identifier.citedreferenceHashizume K. and Chaussidon M. 2005. A non‐terrestrial 16 O‐rich isotopic composition for the protosolar nebula. Nature 434: 619 – 622.en_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


Files in this item

Name:
j.1945-5100.2008.tb00702.x.pdf
Size:
5.031MB
Format:
PDF
View/Open

Show simple item record

Remediation of Harmful Language

The University of Michigan Library aims to describe library materials in a way that respects the people and communities who create, use, and are represented in our collections. Report harmful or offensive language in catalog records, finding aids, or elsewhere in our collections anonymously through our metadata feedback form. More information at Remediation of Harmful Language.

Accessibility

If you are unable to use this file in its current format, please select the Contact Us link and we can modify it to make it more accessible to you.