Show simple item record

dc.creatorThaddeus, P.en_US
dc.creatorGottlieb, C. A.en_US
dc.creatorGupta, H.en_US
dc.creatorBrunken, S.en_US
dc.creatorMcCarthy, M. C.en_US
dc.creatorAgundez, M.en_US
dc.creatorGuelin, M.en_US
dc.creatorCernicharo, J.en_US
dc.date.accessioned2016-04-28T19:36:24Z
dc.date.available2016-04-28T19:36:24Z
dc.date.issued2008-04en
dc.identifierdoi:10.15781/T29N72
dc.identifier.citationThaddeus, P., C. A. Gottlieb, H. Gupta, S. Br�nken, M. C. McCarthy, M. Ag�ndez, M. Gu�lin, and J. Cernicharo. "Laboratory and astronomical detection of the negative molecular ion C3N?." The Astrophysical Journalm, Vol. 677, No. 2 (Apr., 2008): 1132.en_US
dc.identifier.issn0004-637Xen_US
dc.identifier.urihttp://hdl.handle.net/2152/34886
dc.description.abstractThe negative molecular ion C3N- has been detected at millimeter wavelengths in a low-pressure laboratory discharge, and then with frequencies derived from the laboratory data in the molecular envelope of IRC+10216. Spectroscopic constants derived from laboratory measurements of 12 transitions between 97 and 378 GHz allow the rotational spectrum to be calculated well into the submillimeter-wave band to 0.03 km s(-1) or better in equivalent radial velocity. Four transitions of C3N- were detected in IRC+10216 with the IRAM 30 m telescope at precisely the frequencies calculated from the laboratory measurements. The column density of C3N- is 0.5% that of C3N, or approximately 20 times greater than that of C4H- relative to C4H. The C3N- abundance in IRC+10216 is compared with a chemical model calculation by Petrie & Herbst. An upper limit in TMC-1 for C3N- relative to C3N (< 0.8%) and a limit for C4H- relative to C4H (< 0.004%) that is 5 times lower than that found in IRC+10216, were obtained from observations with the NRAO 100 m Green Bank Telescope (GBT). The fairly high concentration ofen_US
dc.description.sponsorshipNRFen_US
dc.description.sponsorshipKorean government MEST 2012R1A1A1014646, 2012M4A2026720en_US
dc.description.sponsorshipSoutheast Physics Network (SEP-Net)en_US
dc.description.sponsorshipScience and Technology Facilities Council ST/F002858/1, ST/I000976/1en_US
dc.description.sponsorshipSwedish Research Council 2009-4088en_US
dc.description.sponsorshipU.S. NSF AST-0708176, AST-1009799en_US
dc.description.sponsorshipNASA NNX07AH09G, NNG04G177G, NNX11AE09Gen_US
dc.description.sponsorshipChandra grant SAO TM8-9009Xen_US
dc.language.isoEnglishen_US
dc.relation.ispartofen_US
dc.rightsAdministrative deposit of works to Texas ScholarWorks: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University.en_US
dc.subjectism : moleculesen_US
dc.subjectline : identificationen_US
dc.subjectmolecular dataen_US
dc.subjectmolecularen_US
dc.subjectprocessesen_US
dc.subjectradio lines : ismen_US
dc.subjectautodetachment spectroscopyen_US
dc.subjectrotational spectraen_US
dc.subjectline surveyen_US
dc.subjectc4hen_US
dc.subjectirc+10216en_US
dc.subjectc8hen_US
dc.subjectradicalsen_US
dc.subjectphotochemistryen_US
dc.subjectattachmenten_US
dc.subjectdynamicsen_US
dc.subjectastronomy & astrophysicsen_US
dc.titleLaboratory And Astronomical Detection Of The Negative Molecular Ion C3N-en_US
dc.typeArticleen_US
dc.description.departmentBiochemistryen_US
dc.identifier.Filename2008_04_c3n-.pdfen_US
dc.rights.restrictionOpenen_US
dc.identifier.doi10.1086/528947en_US
dc.contributor.utaustinauthorAgundez, M.en_US
dc.relation.ispartofserialAstrophysical Journalen_US


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record