Stimulated recombination emission from rapidly cooling regions in an accretion disc and its application to SS 433

Details Stimulated recombination emission from rapidly cooling regions in an accretion disc and its application to SS 433 Stimulated recombination emission from rapidly cooling regions in an accretion disc and its application to SS 433

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.194..177f&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 194, Jan. 1981, p. 177-185.

Astronomy and Astrophysics

Astronomy

7

Black Holes (Astronomy), H Lines, Helium, Lasing, Stellar Mass Accretion, Stimulated Emission, Balmer Series, Binary Stars, Cooling, Red Shift, Stellar Temperature, Temperature Distribution

Scientific paper

The possibility of the recombination lasing mechanism working in a
rapidly cooling ring-like region of an accretion disc around a black
hole is proposed. Such a disc should have coherent line emissions of H
and He I. This model could be used to explain consistently all the
observed facts of SS 433.

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