NASA NTRS · 19720018092
A plausible energy source and structure for quasi-stellar objects
Abstract
If a collision of two large, massive, fast gas clouds occurs, their kinetic energy is converted to radiation in a pair of shock fronts at their interface. The resulting structure is described, and the relevance of this as a radiation source for quasi-stellar objects is considered.
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Daltabuit, E., Cox, D.. 1972-01-01. A plausible energy source and structure for quasi-stellar objects. https://ntrs.nasa.gov/citations/19720018092
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