eFTC-210101

The Physical Nature of Sagittarius A* and The Event Horizon Telescope Data
30 January 2021

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Abstract

The high definition reconstructed pictures of the Messier 87* Active Galactic Nucleus (AGN) from the Event Horizon interferometric Radio-Telescope (EHT) collaboration have boosted up the black hole theory believers. We have instead argued in favor of the identification of this object as a Magnetospheric Eternally Collapsing Object (MECO) with finite luminosity, large but finite redshift and an intrinsic magnetic moment. Here we strongly encourage the EHT research collaboration team to publish whatever collected data they got from Sagitarius A* as the Bondi accretion MECO model of Robertson and Leiter as well as the larger scale disk accretion MECO model of Schild would predict magnetic inflow and outflow patterns in high resolution images distinct from the ones obtained by numerical simulations while treating Sgr A* as a black hole. In particular, sub-millimeter radio pictures of possible funnel flows into the central compact object polar region would provide the MECO theory strong support in addition to the existing 2013 NASA Sofia/Forcast mission far-IR spectacular pictures of a radiating 3-arms structure. Such a structure was identified by Schild as synchrotron radiation from electrons spiraling along the MECO magnetic field lines and originating from the circumnuclear ring (CNR) inner accretion disk toward a polar region of the compact object.

Copyright © 2021 Yvan Leblanc. All rights reserved

PACS: 4.60.+n, 11.17.+y, 97.60.Lf

Cite as: Leblanc, Y., "The Physical Nature of Sagittarius A* and The Event Horizon Telescope Data", manuscript no. eFTC-210101 (2021). http://www.efieldtheory.com/abs/?eFTC-210101; doi:10.13140/RG.2.2.25859.84005.