Radio emission from dark matter annihilation in the Large Magellanic Cloud

Monthly Notices of the Royal Astronomical Society

Volumn 410, Issue 4, 2011, Pages 2463-2471

  Siffert, Beatriz B ^a   Limone, Angelo ^a   Borriello, Enrico ^a,b   Longo, Giuseppe ^a,c,d   Miele, Gennaro ^a,b  

^a UNIVERSITY OF NAPLES FEDERICO II   (Italy)

^b INFN SEZIONE DI NAPOLI   (Italy)

^c INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^d CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Dark matter; Galaxies: individual: Large Magellanic Cloud; Magnetic fields; Radio continuum: galaxies

Indexed keywords

ENERGY DISSIPATION; GALAXIES;

ANNIHILATION SIGNALS; DARK MATTER; GALAXIES: INDIVIDUAL: LARGE MAGELLANIC CLOUDS; MAGNETIC-FIELD; RADIO CONTINUUM: GALAXIES; RADIO EMISSION; RADIOFREQUENCIES; SYNCHROTRON EMISSION; WEAKLY INTERACTING MASSIVE PARTICLES;

MAGNETIC FIELDS;

EID: 78751636416     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.17613.x     Document Type: Article

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