Publication:
Fermi establishes classical novae as a distinct class of gamma-ray sources: The Fermi-LAT collaboration

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dc.contributor.authorM. Ermannen_US
dc.contributor.authorM. Ajelloen_US
dc.contributor.authorA. Alberten_US
dc.contributor.authorL. Baldinien_US
dc.contributor.authorJ. Balleten_US
dc.contributor.authorG. Barbiellinien_US
dc.contributor.authorD. Bastierien_US
dc.contributor.authorR. Bellazzinien_US
dc.contributor.authorE. Bissaldien_US
dc.contributor.authorR. D. Blandforden_US
dc.contributor.authorE. D. Bloomen_US
dc.contributor.authorE. Bottacinien_US
dc.contributor.authorT. J. Brandten_US
dc.contributor.authorJ. Bregeonen_US
dc.contributor.authorP. Bruelen_US
dc.contributor.authorR. Buehleren_US
dc.contributor.authorS. Busonen_US
dc.contributor.authorG. A. Caliandroen_US
dc.contributor.authorR. A. Cameronen_US
dc.contributor.authorM. Caragiuloen_US
dc.contributor.authorP. A. Caraveoen_US
dc.contributor.authorE. Cavazzutien_US
dc.contributor.authorE. Charlesen_US
dc.contributor.authorA. Chekhtmanen_US
dc.contributor.authorC. C. Cheungen_US
dc.contributor.authorJ. Chiangen_US
dc.contributor.authorG. Chiaroen_US
dc.contributor.authorS. Ciprinien_US
dc.contributor.authorR. Clausen_US
dc.contributor.authorJ. Cohen-Tanugien_US
dc.contributor.authorJ. Conraden_US
dc.contributor.authorS. Corbelen_US
dc.contributor.authorF. D'Ammandoen_US
dc.contributor.authorA. De Angelisen_US
dc.contributor.authorP. R. Den Hartogen_US
dc.contributor.authorF. De Palmaen_US
dc.contributor.authorC. D. Dermeren_US
dc.contributor.authorR. Desianteen_US
dc.contributor.authorS. W. Digelen_US
dc.contributor.authorL. Di Venereen_US
dc.contributor.authorE. Do Couto E Silvaen_US
dc.contributor.authorD. Donatoen_US
dc.contributor.authorP. S. Drellen_US
dc.contributor.authorA. Drlica-Wagneren_US
dc.contributor.authorC. Favuzzien_US
dc.contributor.authorE. C. Ferraraen_US
dc.contributor.authorW. B. Fockeen_US
dc.contributor.authorA. Franckowiaken_US
dc.contributor.authorL. Fuhrmannen_US
dc.contributor.authorY. Fukazawaen_US
dc.contributor.authorP. Fuscoen_US
dc.contributor.authorF. Garganoen_US
dc.contributor.authorD. Gasparrinien_US
dc.contributor.authorS. Germanien_US
dc.contributor.authorN. Gigliettoen_US
dc.contributor.authorF. Giordanoen_US
dc.contributor.authorM. Girolettien_US
dc.contributor.authorT. Glanzmanen_US
dc.contributor.authorG. Godfreyen_US
dc.contributor.authorI. A. Grenieren_US
dc.contributor.authorJ. E. Groveen_US
dc.contributor.authorS. Guiriecen_US
dc.contributor.authorD. Hadaschen_US
dc.contributor.authorA. K. Hardingen_US
dc.contributor.authorM. Hayashidaen_US
dc.contributor.authorE. Haysen_US
dc.contributor.authorJ. W. Hewitten_US
dc.contributor.authorA. B. Hillen_US
dc.contributor.authorX. Houen_US
dc.contributor.authorP. Jeanen_US
dc.contributor.authorT. Jogleren_US
dc.contributor.authorG. Jóhannessonen_US
dc.contributor.authorA. S. Johnsonen_US
dc.contributor.authorW. N. Johnsonen_US
dc.contributor.authorM. Kerren_US
dc.contributor.authorJ. Knödlsederen_US
dc.contributor.otherDeutsche Elektronen-Synchrotronen_US
dc.contributor.otherClemson Universityen_US
dc.contributor.otherKavli Institute for Particle Astrophysics and Cosmologyen_US
dc.contributor.otherIstituto Nazionale di Fisica Nucleare, Romaen_US
dc.contributor.otherInstitut de Recherche sur les Lois Fondamentales de l'Universen_US
dc.contributor.otherUniversita degli Studi di Triesteen_US
dc.contributor.otherIstituto Nazionale Di Fisica Nucleare, Sezione di Padovaen_US
dc.contributor.otherUniversita degli Studi di Padovaen_US
dc.contributor.otherNASA Goddard Space Flight Centeren_US
dc.contributor.otherLaboratoire Univers et Particules de Montpellieren_US
dc.contributor.otherLaboratoire Leprince-Ringueten_US
dc.contributor.otherConsorzio Interuniversitario per la Fisica Spaziale (CIFS)en_US
dc.contributor.otherINAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milanen_US
dc.contributor.otherAgenzia Spaziale Italianaen_US
dc.contributor.otherGeorge Mason University, Fairfax Campusen_US
dc.contributor.otherNaval Research Laboratoryen_US
dc.contributor.otherOsservatorio Astronomico di Romaen_US
dc.contributor.otherStockholms universiteten_US
dc.contributor.otherOskar Klein Centre for Cosmoparticle Physicsen_US
dc.contributor.otherK. A. Wallenberg Foundationen_US
dc.contributor.otherKungl. Vetenskapsakademienen_US
dc.contributor.otherInstitut Universitaire de Franceen_US
dc.contributor.otherIstituto Di Radioastronomia, Bolognaen_US
dc.contributor.otherAlma Mater Studiorum Universita di Bolognaen_US
dc.contributor.otherUniversita degli Studi di Udineen_US
dc.contributor.otherUniversita degli Studi di Barien_US
dc.contributor.otherUniversity of Marylanden_US
dc.contributor.otherFermi National Accelerator Laboratoryen_US
dc.contributor.otherMax Planck Institut fur Radioastronomieen_US
dc.contributor.otherHiroshima Universityen_US
dc.contributor.otherUniversita degli Studi di Perugiaen_US
dc.contributor.otherNASA Postdoctoral Program Fellowen_US
dc.contributor.otherMedizinische Universitat Innsbrucken_US
dc.contributor.otherUniversity of Tokyoen_US
dc.contributor.otherUniversity of Maryland, Baltimore Countyen_US
dc.contributor.otherUniversity of Southamptonen_US
dc.contributor.otherMarie Curie IOFen_US
dc.contributor.otherCentre d'Etudes Nucleaires de Bordeaux Gradignanen_US
dc.contributor.otherCNRS Centre National de la Recherche Scientifiqueen_US
dc.contributor.otherUniversite de Toulouseen_US
dc.contributor.otherUniversity Science Institute Reykjaviken_US
dc.contributor.otherAustralia Telescope National Facilityen_US
dc.contributor.otherYale Universityen_US
dc.contributor.otherMahidol Universityen_US
dc.contributor.otherUniversity of California, Irvineen_US
dc.date.accessioned2018-11-09T03:18:24Z
dc.date.available2018-11-09T03:18:24Z
dc.date.issued2014-08-01en_US
dc.description.abstractA classical nova results from runaway thermonuclear explosions on the surface of a white dwarf that accretes matter from a low-mass main-sequence stellar companion. In 2012 and 2013, three novae were detected in γ rays and stood in contrast to the first γ-ray-detected nova V407 Cygni 2010, which belongs to a rare class of symbiotic binary systems. Despite likely differences in the compositions and masses of their white dwarf progenitors, the three classical novae are similarly characterized as soft-spectrum transient γ-ray sources detected over 2- to 3-week durations. The γ-ray detections point to unexpected high-energy particle acceleration processes linked to the mass ejection from thermonuclear explosions in an unanticipated class of Galactic γ-ray sources.en_US
dc.identifier.citationScience. Vol.345, No.6196 (2014), 554-558en_US
dc.identifier.doi10.1126/science.1253947en_US
dc.identifier.issn10959203en_US
dc.identifier.issn00368075en_US
dc.identifier.other2-s2.0-84905901421en_US
dc.identifier.urihttps://repository.li.mahidol.ac.th/handle/123456789/34969
dc.rightsMahidol Universityen_US
dc.rights.holderSCOPUSen_US
dc.source.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=84905901421&origin=inwarden_US
dc.subjectMultidisciplinaryen_US
dc.titleFermi establishes classical novae as a distinct class of gamma-ray sources: The Fermi-LAT collaborationen_US
dc.typeArticleen_US
dspace.entity.typePublication
mu.datasource.scopushttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=84905901421&origin=inwarden_US

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