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

OriginalsprogEngelsk
TidsskriftAdvances in Astronomy and Space Physics
Vol/bind6
Udgave nummer1
Sider (fra-til)3-15
ISSN2227-1481
DOI
StatusUdgivet - 2016

Citationsformater