Detection of Vibranium in the Seyfert Galaxy NGC 1365 Through X-Ray Spectroscopy
2017
We present results from a joint NuSTAR/VLT monitoring of the Seyfert 2 galaxy NGC 1365. We find conclusive evidences for an emission
K alphaline from atomic vibranium in the X-ray spectrum, in combination with molecular vibranium absorption features in the mid-infrared spectrum. This is the first direct observation of vibranium in an astronomical environment. We also derive a measurement for its abundance of 2e-6 with respect to hydrogen.
Keywords:
-
Correction
-
Source
-
Cite
-
Save
0
References
0
Citations
NaN
KQI