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Observation of the new emission line at similar to 3.5 keV in the X-ray spectra of galaxies and galaxy clusters. / Iakubovskyi, D. A.
I:
Advances in Astronomy and Space Physics, Bind 6, Nr. 1, 2016, s. 3-15.
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Harvard
Iakubovskyi, DA 2016, '
Observation of the new emission line at similar to 3.5 keV in the X-ray spectra of galaxies and galaxy clusters',
Advances in Astronomy and Space Physics, bind 6, nr. 1, s. 3-15.
https://doi.org/10.17721/2227-1481.6.3-15APA
Iakubovskyi, D. A. (2016).
Observation of the new emission line at similar to 3.5 keV in the X-ray spectra of galaxies and galaxy clusters.
Advances in Astronomy and Space Physics,
6(1), 3-15.
https://doi.org/10.17721/2227-1481.6.3-15Vancouver
Iakubovskyi DA.
Observation of the new emission line at similar to 3.5 keV in the X-ray spectra of galaxies and galaxy clusters.
Advances in Astronomy and Space Physics. 2016;6(1):3-15.
https://doi.org/10.17721/2227-1481.6.3-15Author
Iakubovskyi, D. A. / Observation of the new emission line at similar to 3.5 keV in the X-ray spectra of galaxies and galaxy clusters. I: Advances in Astronomy and Space Physics. 2016 ; Bind 6, Nr. 1. s. 3-15.
Bibtex
@article{3d76e976dcf449d6bced62f85fd14f7e,
title = "Observation of the new emission line at similar to 3.5 keV in the X-ray spectra of galaxies and galaxy clusters",
keywords = "X-rays: general, dark matter, line: identification",
author = "Iakubovskyi, {D. A.}",
year = "2016",
doi = "10.17721/2227-1481.6.3-15",
language = "English",
volume = "6",
pages = "3--15",
journal = "Advances in Astronomy and Space Physics",
issn = "2227-1481",
number = "1",
}
RIS
TY - JOUR
T1 - Observation of the new emission line at similar to 3.5 keV in the X-ray spectra of galaxies and galaxy clusters
AU - Iakubovskyi, D. A.
PY - 2016
Y1 - 2016
KW - X-rays: general
KW - dark matter
KW - line: identification
U2 - 10.17721/2227-1481.6.3-15
DO - 10.17721/2227-1481.6.3-15
M3 - Journal article
VL - 6
SP - 3
EP - 15
JO - Advances in Astronomy and Space Physics
JF - Advances in Astronomy and Space Physics
SN - 2227-1481
IS - 1
ER -
