Is MC22 a Neutron Star or a Black Hole?

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MC22 is a bright astronomical source emitting at L=10^31W, but lacks rapid periodic pulsations in its X-ray flux, complicating its classification. The emission is likely due to material accretion from a star, suggesting it could be either a neutron star or a black hole. The discussion seeks to determine if one or both possibilities can be conclusively excluded based on the available data. Additionally, questions arise about the object's mass, reality, and dimensions. Clarifying these aspects is crucial for understanding the nature of MC22.
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Can anyone help please,

MC22 is a very bright source, radiating at L=10^31W. However, no rapid periodic pulsations are apparent in the X-ray flux. It suggested that this emission arises from accretion of material from a star onto either a neutron star or black hole. From these facts can you conclusively exclude neither, one or both of these possibilities? Show how you arrived at your answer.

Any help would be great,

thank you Col.
 
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