Identification of the ~3.55 keV emission line candidate objects across the sky
An emission line at the energy ∼3.55 keV detected in different galaxies and galaxy clusters has caused numerous discussions in high-energy astrophysics and particle physics communities. To reveal the origin of the line, we analyzed publicly-available observations of MOS cameras from XMM-Newton cosmi...
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| Date: | 2015 |
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| Main Authors: | , |
| Format: | Article |
| Language: | English |
| Published: |
Головна астрономічна обсерваторія НАН України
2015
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| Series: | Advances in Astronomy and Space Physics |
| Online Access: | http://dspace.nbuv.gov.ua/handle/123456789/119931 |
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| Journal Title: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Cite this: | Identification of the ~3.55 keV emission line candidate objects across the sky / D.O. Savchenko, D.A. Iakubovskyi // Advances in Astronomy and Space Physics. — 2015. — Т. 5., вип. 2. — С. 89-92. — Бібліогр.: 24 назв. — англ. |