Cobalt-56 γ 3-ray emission lines from the type Ia supernova 2014J

Nature

Volumn 512, Issue 7515, 2014, Pages 406-408

  Churazov, E ^a,b   Sunyaev, R ^a,b   Isern, J ^c   Knodlseder J ^d,e   Jean, P ^d,e   Lebrun, F ^f   Chugai, N ^g   Grebenev, S ^a   Bravo, E ^h   Sazonov, S ^a,i   Renaud, M ^j  

^a Space Research Institute ^*  (Russian Federation)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^c CSIC   (Spain)

^d OBSERVATOIRE MIDI PYRÉNÉES   (France)

^e IRAP   (France)

^f UNIVERSITÉ PARIS DESCARTES   (France)

^g INSTITUTE OF ASTRONOMY   (Russian Federation)

^h UNIVERSITAT POLITÈCNICA DE CATALUNYA   (Spain)

ⁱ MOSCOW INSTITUTE OF PHYSICS AND TECHNOLOGY   (Russian Federation)

^j UNIV MONTPELLIER   (France)

more..

Author keywords

[No Author keywords available]

Indexed keywords

COBALT; COBALT 56; NICKEL 56; RADIOISOTOPE; UNCLASSIFIED DRUG;

COBALT; EXPLOSION; EXTRATERRESTRIAL MATTER; GAMMA RAY RADIATION; GRAVITY;

ARTICLE; BREMS RADIATION; COLLAPSE; COMPTON EFFECT; DWARFISM; EXPLOSION; GAMMA RADIATION; GRAVITY; LUMINANCE; NUCLEAR ENERGY; NULL HYPOTHESIS; PRIORITY JOURNAL; SIGNAL NOISE RATIO; TYPE IA SUPERNOVA; VELOCITY;

EID: 84907411083     PISSN: 00280836     EISSN: 14764687     Source Type: Journal    
DOI: 10.1038/nature13672     Document Type: Article

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