Raman scattering as a diagnostic possibility in astrophysics

Details Raman scattering as a diagnostic possibility in astrophysics Raman scattering as a diagnostic possibility in astrophysics

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...211l..27n&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 211, no. 2, March 1989, p. L27-L30. Research supported by SNSF.

Astronomy and Astrophysics

Astrophysics

60

Astronomical Spectroscopy, Plasma Diagnostics, Raman Spectra, Seyfert Galaxies, Galactic Nuclei, High Temperature Plasmas, Iron, Nebulae, Rayleigh Scattering, Spectral Line Width

Scientific paper

It is shown that Raman scattering deserves to be included in the
diagnostic tools of the spectroscopy of gaseous nebulae and emission
regions of galactic nuclei. It is pointed out that Raman scattering may
be the source of some up to now unidentified emission lines. It is shown
that Raman scattering may act as a line-broadening mechanism.

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