Further Evidence for Raman Scattering in Rr-Telescopii

Details Further Evidence for Raman Scattering in Rr-Telescopii Further Evidence for Raman Scattering in Rr-Telescopii

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.264..975v&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 264, NO. 4/OCT15, P. 975, 1993

Astronomy and Astrophysics

Astronomy

22

Line: Identification - Scattering - Stars: Emission-Line, Be - Stars: Individual: Rr Tel

Scientific paper

Raman scattering of O VI λλ1302, 1308 photons on the ground level of neutral hydrogen has been suggested as the cause of the broad emission features at 6825 and 7088 Å in the spectra of symbiotic stars. We report on the detection of other Raman lines in the optical spectrum of the symbiotic star RR Tel. The lines detected are two He II Balmer lines that are Raman-scattered to wavelengths close to hydrogen Hβ and Hγ. Another possible detection is scattered C III λ977, which appears at about 4977 Å in the optical spectrum.

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