The quasar 0805 + 046 as a helium-rich shell star

Details The quasar 0805 + 046 as a helium-rich shell star The quasar 0805 + 046 as a helium-rich shell star

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.117..337v&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 117, no. 2, Dec. 1985, p. 337-350.

Astronomy and Astrophysics

Astrophysics

2

Helium, Quasars, Shell Stars, Stellar Envelopes, Stellar Models, Absorption Spectra, Emission Spectra, Lasing, Line Spectra

Scientific paper

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. (1) The strong emission line at 4712 Å is identified with He I λ4713. (2) The discontinuity in the continuous energy distribution at λ3420 is identified with the helium discontinuity at λ3422. (3) 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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