Publication:
Formation of anionic c, n-bearing chains in the interstellar medium via reactions of h- with hcxn for odd-valued x from 1 to 7

dc.contributor.coauthorGianturco, F. A.
dc.contributor.coauthorSatta, M.
dc.contributor.coauthorWester, R.
dc.contributor.departmentDepartment of Chemistry
dc.contributor.kuauthorYurtsever, İsmail Ersin
dc.contributor.kuprofileFaculty Member
dc.contributor.otherDepartment of Chemistry
dc.contributor.schoolcollegeinstituteCollege of Sciences
dc.contributor.yokid7129
dc.date.accessioned2024-11-09T13:23:14Z
dc.date.issued2017
dc.description.abstractStudy Design: A retrospective study investigating decrease in the nucleus pulposus signal intensity or disc height on magnetic resonance imaging (MRI) and disc degeneration. Purpose: Although a degenerated disc cannot self- regenerate, distraction or stabilization may provide suitable conditions for rehydration and possible regeneration. This study aimed to evaluate clinical outcomes and disc regeneration via MRI in a series of patients with degenerative disc disease (DDD) who underwent lumbar stabilization with a dynamic stabilization system (DSS). Overview of Literature: A dynamic system provides rehydration during early DDD. Methods: Fifty- nine patients (mean age, 46.5 years) who undedwent stabilization with DSS for segmental instability (painful black disc) between 2004 and 2014 were retrospectively evaluated. All patients underwent MRI preoperatively and 12 months postoperatively. Intervertebral disc (IVD) degeneration grades at the implanted segment were categorized using the Pfirrmann classification system. Patients were followed for a mean of 6.4 years, and clinical outcomes were based on visual analog scale (VAS) and Oswestry disability index (ODI) scores. Results: Significant improvements in back pain VAS and ODI scores from before surgery (7 and 68%, respectively) were reported at 6 (2.85 and 27.4%, respectively) and 12 months postoperatively (1.8 and 16.3%, respectively). Postoperative IVD changes were observed in 28 patients. Improvement was observed in 20 patients (34%), whereas progressive degeneration was observed in eight patients (13.5%). Thirty- one patients (52.5%) exhibited neither improvement nor progression. Single Pfirrmann grade improvements were observed in 29% of the patients and two- grade improvements were observed in 5%. Conclusions: Our observations support the theory that physiological movement and a balanced load distribution are necessary for disc regeneration. We conclude that DSS may decelerate the degeneration process and appears to facilitate regeneration.
dc.description.fulltextYES
dc.description.indexedbyWoS
dc.description.indexedbyScopus
dc.description.issue1
dc.description.openaccessYES
dc.description.publisherscopeInternational
dc.description.sponsoredbyTubitakEuN/A
dc.description.sponsorshipAustrian Science Fund (FWF)
dc.description.versionPublisher version
dc.description.volume850
dc.formatpdf
dc.identifier.doi10.3847/1538-4357/aa92ca
dc.identifier.eissn1538-4357
dc.identifier.embargoNO
dc.identifier.filenameinventorynoIR01208
dc.identifier.issn0004-637X
dc.identifier.linkhttps://doi.org/10.3847/1538-4357/aa92ca
dc.identifier.quartileQ1
dc.identifier.scopus2-s2.0-85037686428
dc.identifier.urihttps://hdl.handle.net/20.500.14288/3361
dc.identifier.wos415597600004
dc.keywordsAstrochemistry
dc.keywordsISM: clouds
dc.keywordsISM: molecules
dc.keywordsISM: planetary nebulae
dc.keywordsMolecular processes
dc.languageEnglish
dc.publisherAmerican Astronomical Society (AAS)
dc.relation.grantnoP27047-N20
dc.relation.urihttp://cdm21054.contentdm.oclc.org/cdm/ref/collection/IR/id/2393
dc.sourceAstrophysical Journal
dc.subjectChemistry
dc.subjectAstronomy and astrophysics
dc.titleFormation of anionic c, n-bearing chains in the interstellar medium via reactions of h- with hcxn for odd-valued x from 1 to 7
dc.typeJournal Article
dspace.entity.typePublication
local.contributor.authorid0000-0001-9245-9596
local.contributor.kuauthorYurtsever, İsmail Ersin
relation.isOrgUnitOfPublication035d8150-86c9-4107-af16-a6f0a4d538eb
relation.isOrgUnitOfPublication.latestForDiscovery035d8150-86c9-4107-af16-a6f0a4d538eb

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