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New emission line at ~3.5 keV - observational status, connection with radiatively decaying dark matter and directions for future studies

Recent works of Bulbul et al. (2014) and Boyarsky et al. (2014), claiming the detection of the extra emission line with energy ∼3.5 keV in X-ray spectra of certain clusters of galaxies and nearby Andromeda galaxy, have raised a considerable interest in astrophysics and particle physics communities....

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Veröffentlicht in:Advances in Astronomy and Space Physics
Datum:2014
1. Verfasser: Iakubovskyi, D.A.
Format: Artikel
Sprache:Englisch
Veröffentlicht: Головна астрономічна обсерваторія НАН України 2014
Online Zugang:https://nasplib.isofts.kiev.ua/handle/123456789/119805
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Zitieren:New emission line at ~3.5 keV - observational status, connection with radiatively decaying dark matter and directions for future studies / D.A. Iakubovskyi // Advances in Astronomy and Space Physics. — 2014. — Т. 4., вип. 1-2. — С. 9-14. — Бібліогр.: 98 назв. — англ.

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