Adiabatic deceleration of secondary antiprotons in the envelopes of supernova exploding in dense clouds |
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Authors: | S A Stephens B G Mauger |
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Institution: | (1) Department of Physics, University of Ottawa, K1N 6N5, Canada |
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Abstract: | Within the framework of the plasma-laser star model of quasars it is proposed that the quasar 0805+046 is a helium-rich shell star. (a) The strong emission line at 4712 Å is identified with Hei 4713. (b) The discontinuity in the continuous energy distribution at 3420 is identified with the helium discontinuity at 3422. (c) In the absorption-line spectrum many lines have been identified. It is shown that the proposed model provides a consistent and satisfactory interpretation of the observed spectra. |
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