Raman spectra of the T Tauri star LkHα 120

Details Raman spectra of the T Tauri star LkHα 120 Raman spectra of the T Tauri star LkHα 120

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acasn..33....1c&link_type=abstract

Acta Astronomica Sinica (ISSN 0001-5245), vol. 33, no. 1, March 1992, p. 1-4. In Chinese.

Astronomy and Astrophysics

Astrophysics

Raman Spectra, Stellar Spectra, T Tauri Stars, Emission Spectra, Stellar Spectrophotometry

Scientific paper

Raman scattering was successfully used to interpret some unidentified emission lines. This shows that Raman scattering may play an important role in astrophysics. The cross-section and line intensities of Raman scattering are estimated and almost all the unidentified emission lines of the T Tauri star LkHα120 (4200.9, 5098.1, 5613.9, 5768.0, 5859.0, 6633.5, 6667.0, 7500.0) are interpreted as Raman-scattered FeI and FeII lines by H, H2, and CO without any assumptions or parameters.

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