Authors: Stefano Sello
The “Event Horizon Telescope”, EHT, is a radio-telescope planetary network, and its goal is to reach a sufficiently high spatial resolution to obtain real images of Sgr A*, a supermassive black hole located at the core of our galaxy. Waiting for real observational data, now we can analyze predicted EHT data obtained from a simulations to "see" the event horizon and the neighborhood of Sgr A*. In this brief research note we suggest a method to improve the capabilities of our current image analyses, using a proper isometric pesudo-3D projection analysis. In fact, the details obtained are impressive and this first result suggests that the pseudo-3D isometric projection analysis could be a useful tool to better study the main properties of the surroundings of the event horizon of a black hole.
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[v1] 2016-07-19 04:22:35
[v2] 2016-07-19 09:11:02
[v3] 2016-07-21 04:20:06
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