Difference between revisions of "Superluminal Flares: Can They Provide the Answer?"
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There have been recent reports of flares at speeds of about 0.9 emanating in opposite directions from a small black hole or quasar within our galaxy. A quirk of geometry causes such flares to appear to be super1uminal. These reports might encourage the investigation of pairs of such flares associated with very distant quasars, thus opening the possibility of solving possible problems regarding the accepted interpretation of red shift data from distant bodies. | There have been recent reports of flares at speeds of about 0.9 emanating in opposite directions from a small black hole or quasar within our galaxy. A quirk of geometry causes such flares to appear to be super1uminal. These reports might encourage the investigation of pairs of such flares associated with very distant quasars, thus opening the possibility of solving possible problems regarding the accepted interpretation of red shift data from distant bodies. | ||
| − | [[Category:Scientific Paper]] | + | [[Category:Scientific Paper|superluminal flares provide answer]] |
Latest revision as of 11:07, 1 January 2017
| Scientific Paper | |
|---|---|
| Title | Superluminal Flares: Can They Provide the Answer? |
| Author(s) | William C Mitchell |
| Keywords | Superluminal Flares |
| Published | 1998 |
| Journal | None |
Abstract
There have been recent reports of flares at speeds of about 0.9 emanating in opposite directions from a small black hole or quasar within our galaxy. A quirk of geometry causes such flares to appear to be super1uminal. These reports might encourage the investigation of pairs of such flares associated with very distant quasars, thus opening the possibility of solving possible problems regarding the accepted interpretation of red shift data from distant bodies.
