Observation of the new emission line at similar to 3.5 keV in the X-ray spectra of galaxies and galaxy clusters

D. A. Iakubovskyi

Original languageEnglish
JournalAdvances in Astronomy and Space Physics
Volume6
Issue number1
Pages (from-to)3-15
ISSN2227-1481
DOIs
Publication statusPublished - 2016

Keywords

  • X-rays: general
  • dark matter
  • line: identification

Cite this